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3. The Probabilistic Solar Particle Event foRecasting (PROSPER) Model

Author

Papaioannou, Athanasios, Vainio, Rami, Raukunen, Osku, Jiggens, Piers, Aran, Angels, Dierckxsens, Mark, Mallios, Sotirios A., Paassilta, Miikka, and Anastasiadis, Anastasios

Subjects
Astrophysics - Solar and Stellar Astrophysics, Physics - Space Physics
Abstract

The Probabilistic Solar Particle Event foRecasting (PROSPER) model predicts the probability of occurrence and the expected peak flux of Solar Energetic Particle (SEP) events. Predictions are derived for a set of integral proton energies (i.e. E$>$10, $>$30 and $>$100 MeV) from characteristics of solar flares (longitude, magnitude), coronal mass ejections (width, speed) and combinations of both. Herein the PROSPER model methodology for deriving the SEP event forecasts is described and the validation of the model, based on archived data, is presented for a set of case studies. The PROSPER model has been incorporated into the new operational Advanced Solar Particle Event Casting System (ASPECS) tool to provide nowcasting (short term forecasting) of SEP events as part of ESA's future SEP Advanced Warning System (SAWS). ASPECS also provides the capability to interrogate PROSPER for historical cases via a run on demand functionality., Comment: Submitted to J. Space Weather & Space Climate

Published
2022

6. Propagating Conditions and the Time of ICMEs Arrival: A Comparison of the Effective Acceleration Model with ENLIL and DBEM Models

Author

Paouris, Evangelos, Calogovic, Jasa, Dumbovic, Mateja, Mays, M. Leila, Vourlidas, Angelos, Papaioannou, Athanasios, Anastasiadis, Anastasios, and Balasis, Georgios

Subjects
Physics - Space Physics
Abstract

The Effective Acceleration Model (EAM) predicts the Time-of-Arrival (ToA) of the Coronal Mass Ejection (CME) driven shock and the average speed within the sheath at 1 AU. The model is based on the assumption that the ambient solar wind interacts with the interplanetary CME (ICME) resulting in constant acceleration or deceleration. The upgraded version of the model (EAMv3), presented here, incorporates two basic improvements: (a) a new technique for the calculation of the acceleration (or deceleration) of the ICME from the Sun to 1 AU and (b) a correction for the CME plane-of-sky speed. A validation of the upgraded EAM model is performed via comparisons to predictions from the ensemble version of the Drag-Based model (DBEM) and the WSA-ENLIL+Cone ensemble model. A common sample of 16 CMEs/ICMEs, in 2013-2014, is used for the comparison. Basic performance metrics such as the mean absolute error (MAE), mean error (ME) and root mean squared error (RMSE) between observed and predicted values of ToA are presented. MAE for EAM model was 8.7$\pm$1.6 hours while for DBEM and ENLIL was 14.3$\pm$2.2 and 12.8$\pm$1.7 hours, respectively. ME for EAM was -1.4$\pm$2.7 hours in contrast with -9.7$\pm$3.4 and -6.1$\pm$3.3 hours from DBEM and ENLIL. We also study the hypothesis of stronger deceleration in the interplanetary (IP) space utilizing the EAMv3 and DBEM models. In particularly, the DBEM model perform better when a greater value of drag parameter, of order of a factor of 3, is used in contrast to previous studies. EAMv3 model shows a deceleration of ICMEs at greater distances, with a mean value of 0.72 AU., Comment: 18 pages, 3 figures, 4 Tables. Accepted in Solar Physics

Published
2020
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7. Assessing the projection correction of Coronal Mass Ejection speeds on Time-of-Arrival prediction performance using the Effective Acceleration Model

Author

Paouris, Evangelos, Vourlidas, Angelos, Papaioannou, Athanasios, and Anastasiadis, Anastasios

Subjects
Astrophysics - Solar and Stellar Astrophysics, Physics - Space Physics
Abstract

White light images of Coronal Mass Ejections (CMEs) are projections on the plane-of-sky (POS). As a result, CME kinematics are subject to projection effects. The error in the true (deprojected) speed of CMEs is one of the main causes of uncertainty to Space Weather forecasts, since all estimates of the CME Time-of-Arrival (ToA) at a certain location within the heliosphere require, as input, the CME speed. We use single viewpoint observations for 1037 flare-CME events between 1996-2017 and propose a new approach for the correction of the CME speed assuming radial propagation from the flare site. Our method is uniquely capable to produce physically reasonable deprojected speeds across the full range of source longitudes. We bound the uncertainty in the deprojected speed estimates via limits in the true angular width of a CME based on multiview-point observations. Our corrections range up to 1.37-2.86 for CMEs originating from the center of the disk. On average, the deprojected speeds are 12.8% greater than their POS speeds. For slow CMEs (VPOS < 400 km/s) the full ice-cream cone model performs better while for fast and very fast CMEs (VPOS > 700 km/s) the shallow ice-cream model gives much better results. CMEs with 691-878 km/s POS speeds have a minimum ToA mean absolute error (MAE) of 11.6 hours. This method, is robust, easy to use, and has immediate applicability to Space Weather forecasting applications. Moreover, regarding the speed of CMEs, our work suggests that single viewpoint observations are generally reliable., Comment: Paper accepted by Space Weather journal

Published
2020
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8. Prediction of solar energetic events impacting space weather conditions

Author

Georgoulis, Manolis K., Yardley, Stephanie L., Guerra, Jordan A., Murray, Sophie A., Ahmadzadeh, Azim, Anastasiadis, Anastasios, Angryk, Rafal, Aydin, Berkay, Banerjee, Dipankar, Barnes, Graham, Bemporad, Alessandro, Benvenuto, Federico, Bloomfield, D. Shaun, Bobra, Monica, Campi, Cristina, Camporeale, Enrico, DeForest, Craig E., Emslie, A. Gordon, Falconer, David, Feng, Li, Gan, Weiqun, Green, Lucie M., Guastavino, Sabrina, Hapgood, Mike, Kempton, Dustin, Kitiashvili, Irina, Kontogiannis, Ioannis, Korsos, Marianna B., Leka, K.D., Massa, Paolo, Massone, Anna Maria, Nandy, Dibyendu, Nindos, Alexander, Papaioannou, Athanasios, Park, Sung-Hong, Patsourakos, Spiros, Piana, Michele, Rawafi, Nour E., Sadykov, Viacheslav M., Toriumi, Shin, Vourlidas, Angelos, Wang, Haimin, L. Wang, Jason T., Whitman, Kathryn, Yan, Yihua, and Zhukov, Andrei N.

Published
2024
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9. The ‘Mini-Jupette’ technique for climacturia: a systematic review

Author

Mykoniatis Ioannis, Tsiakaras Stavros, Savvides Eliophotos, Langas Georgios, Anastasiadis Anastasios, Koenraad van Renterghem, and Andrianne Robert

Subjects
Diseases of the genitourinary system. Urology, RC870-923
Abstract

Background: The leakage of urine during sexual arousal, known as climacturia, is an under-recognized clinical condition often overshadowed by erectile dysfunction in men who have undergone radical prostatectomy. Objectives: This study aims to determine and evaluate the role of the Mini-Jupette technique and its alternatives in the treatment of climacturia. Data sources and methods: We conducted a systematic review following the Preferred Reporting Items for Systematic Reviews and Meta-Analyses guidelines for systematic reviews. We searched Medline via PubMed, Scopus, and the Cochrane Library databases until October 2022. Results: We included seven studies involving 120 patients with climacturia. Different types of grafts were used, ranging from synthetic mesh to autologous grafts. In all seven studies, the use of the Adrianne Mini-Jupette (AMJ) and its alternatives showed a high percentage of improvement in climacturia, with reported complete resolution ranging from 65% to 93%. Regarding postoperative complications, one study reported the highest sling explantation rate at 11% (4/38), while other studies reported complications ranging from subjective symptoms such as dysuria and perineal pain to the need for subsequent artificial urinary sphincter placement. Conclusion: The AMJ sling and its variations are low-cost, time-efficient, and relatively safe procedures with high patient satisfaction rates among those treated for climacturia.

Published
2023
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10. Sources of Solar Energetic Particles

Author

Vlahos, Loukas, Anastasiadis, Anastasios, Papaioannou, Athanasios, Kouloumvakos, Athanasios, and Isliker, Heinz

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

Solar Energetic Particles (SEP) are an integral part of the physical processes related with Space Weather. We present a review for the acceleration mechanisms related to the explosive phenomena (flares and/or CMEs) inside the solar corona. For more than 40 years, the main 2D cartoon representing our understanding of the explosive phenomena inside the solar corona remained almost unchanged. The acceleration mechanisms related to solar flares and CMEs also remained unchanged and were part of the same cartoon. In this review, we revise the standard cartoon and present evidence from recent global MHD simulations that supports the argument that explosive phenomena will lead to the spontaneous formation of current sheets in different parts of the erupting magnetic structure. The evolution of the large scale current sheets and their fragmentation will lead to strong turbulence and turbulent reconnection during solar flares and turbulent shocks. In other words, the acceleration mechanism in flares and CME-driven shocks may be the same, and their difference will be the overall magnetic topology, the ambient plasma parameters, and the duration of the unstable driver., Comment: Accepted at Philosophical Transactions A, 2019

Published
2019
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12. Numerical Simulation of Real-Scale Vibration Experiments of a Steel Frame Structure on a Shallow Foundation

Author

Koronides, Marios, Kontoe, Stavroula, Zdravković, Lidija, Vratsikidis, Athanasios, Pitilakis, Dimitris, Anastasiadis, Anastasios, Potts, David M., Ansal, Atilla, Series Editor, Bommer, Julian, Editorial Board Member, Bray, Jonathan D., Editorial Board Member, Pitilakis, Kyriazis, Editorial Board Member, Yasuda, Susumu, Editorial Board Member, Wang, Lanmin, editor, Zhang, Jian-Min, editor, and Wang, Rui, editor

Published
2022
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13. Small to Medium Strain Dynamic Properties of Lanzhou Loess

Author

Song, Binghui, Tsinaris, Angelos, Anastasiadis, Anastasios, Pitilakis, Kyriazis, Chen, Wenwu, Ansal, Atilla, Series Editor, Bommer, Julian, Editorial Board Member, Bray, Jonathan D., Editorial Board Member, Pitilakis, Kyriazis, Editorial Board Member, Yasuda, Susumu, Editorial Board Member, Wang, Lanmin, editor, Zhang, Jian-Min, editor, and Wang, Rui, editor

Published
2022
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16. Particle Acceleration and Fractional Transport in Turbulent Reconnection

Author

Isliker, Heinz, Pisokas, Theophilos, Vlahos, Loukas, and Anastasiadis, Anastasios

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

We consider a large scale environment of turbulent reconnection that is fragmented into a number of randomly distributed Unstable Current Sheets (UCS), and we statistically analyze the acceleration of particles within this environment. We address two important cases of acceleration mechanisms when the particles interact with the UCS: (a) electric field acceleration, and (b) acceleration through reflection at contracting islands. Electrons and ions are accelerated very efficiently, attaining an energy distribution of power-law shape with an index $1-2$, depending on the acceleration mechanism. The transport coefficients in energy space are estimated from the test-particle simulation data, and we show that the classical Fokker-Planck (FP) equation fails to reproduce the simulation results when the transport coefficients are inserted into it and it is solved numerically. The cause for this failure is that the particles perform Levy flights in energy space, the distributions of energy increments exhibit power-law tails. We then use the fractional transport equation (FTE) derived by Isliker et al., 2017, whose parameters and the order of the fractional derivatives are inferred from the simulation data, and, solving the FTE numerically, we show that the FTE successfully reproduces the kinetic energy distribution of the test-particles. We discuss in detail the analysis of the simulation data and the criteria that allow judging the appropriateness of either an FTE or a classical FP equation as a transport model., Comment: in press at Astrophysical Journal, 2017 (17 pages,22 figures)

Published
2017
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19. Full-Scale Testing of a Structure on Improved Soil Replaced with Rubber–Gravel Mixtures

Author

Vratsikidis, Athanasios, Tsinaris, Angelos, Kapouniaris, Anastasios, Anastasiadis, Anastasios, Pitilakis, Dimitris, Pitilakis, Kyriazis, di Prisco, Marco, Series Editor, Chen, Sheng-Hong, Series Editor, Vayas, Ioannis, Series Editor, Kumar Shukla, Sanjay, Series Editor, Sharma, Anuj, Series Editor, Kumar, Nagesh, Series Editor, Wang, Chien Ming, Series Editor, Hazarika, Hemanta, editor, Madabhushi, Gopal Santana Phani, editor, Yasuhara, Kazuya, editor, and Bergado, Dennes T., editor

Published
2021
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20. Stochastic Fermi Energization of Coronal Plasma during explosive magnetic energy release

Author

Pisokas, Theophilos, Vlahos, Loukas, Isliker, Heinz, Tsiolis, Vassilios, and Anastasiadis, Anastasios

Subjects
Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics
Abstract

The aim of this study is to analyze the interaction of charged particles (ions and electrons) with randomly formed particle scatterers (e.g.\ large scale local "magnetic fluctuations" or "coherent magnetic irregularities"), using the set up proposed initially by \cite{Fermi49}. These scatterers are formed by the explosive magnetic energy release and propagate with the Alfv\'en speed along the irregular magnetic fields. They are large scale local fluctuations ($\delta B/B \approx 1$), randomly distributed inside the unstable magnetic topology and will here be called {\bf Alfv\'enic Scatterers (AS)}. We constructed a 3D grid on which a small fraction of randomly chosen grid points are acting as AS. In particular, we study how a large number of test particles evolve inside a collection of AS, analyzing the evolution of their energy distribution and their escape time distribution. We use a well established method to estimate the transport coefficients directly from the trajectories of the particles. Using the estimated transport coefficients and solving the Fokker-Planck (FP) equation numerically, we can recover the energy distribution of the particles. We have shown that the Stochastic Fermi Energization (SFE) of mildly relativistic and relativistic plasma can heat and accelerate the tail of the ambient particle distribution as predicted by \citet{Parker58} and \citet{Ramaty79}. The temperature of the hot plasma and the tail of the energetic particles depend on the mean free path ($\lambda_{\rm sc}$) of the particles between the scatterers inside the energization volume., Comment: 30 pages, 25 figures. Accepted for publication in the Astrophysical Journal (2016)

Published
2016
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21. Particle Acceleration and Heating by Turbulent Reconnection

Author

Vlahos, Loukas, Pisokas, Theophilos, Isliker, Heinz, Tsiolis, Vassilios, and Anastasiadis, Anastasios

Subjects
Astrophysics - Solar and Stellar Astrophysics, Physics - Plasma Physics
Abstract

Turbulent flows in the solar wind, large scale current sheets, multiple current sheets, and shock waves lead to the formation of environments in which a dense network of current sheets is established and sustains "turbulent reconnection". We constructed a 2D grid on which a number of randomly chosen grid points are acting as scatterers (i.e. magnetic clouds or current sheets). Our goal is to examine how test particles respond inside this large scale collection of scatterers. We study the energy gain of individual particles, the evolution of their energy distribution and their escape time distribution. We have developed a new method to estimate the transport coefficients from the dynamics of the interaction of the particles with the scatterers. Replacing the "magnetic clouds" with current sheets, we have proven that the energization processes can be more efficient depending on the strength of the effective electric fields inside the current sheets and their statistical properties. Using the estimated transport coefficients and solving the Fokker-Planck (FP) equation we can recover the energy distribution of the particles only for the sstochastic Fermi process. We have shown that the evolution of the particles inside a turbulent reconnecting volume is not a solution of the FP equation, since the interaction of the particles with the current sheets is "anomalous", in contrast to the case of the second order Fermi process., Comment: 6 pages, 8 figures, in press at Astrophysical Journal Letters (2016)

Published
2016
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23. Accurately specifying storm-time ULF wave radial diffusion in the radiation belts

Author

Dimitrakoudis, Stavros, Mann, Ian R., Balasis, Georgios, Papadimitriou, Constantinos, Anastasiadis, Anastasios, and Daglis, Ioannis A.

Subjects
Physics - Space Physics
Abstract

Ultra-low frequency (ULF) waves can contribute to the transport, acceleration and loss of electrons in the radiation belts through inward and outward diffusion. However, the most appropriate parameters to use to specify the ULF wave diffusion rates are unknown. Empirical representations of diffusion coefficients often use Kp; however, specifications using ULF wave power offer an improved physics-based approach. We use 11 years of ground-based magnetometer array measurements to statistically parameterise the ULF wave power with Kp, solar wind speed, solar wind dynamic pressure and Dst. We find Kp is the best single parameter to specify the statistical ULF wave power driving radial diffusion. Significantly, remarkable high energy tails exist in the ULF wave power distributions when expressed as a function of Dst. Two parameter ULF wave power specifications using Dst as well as Kp provide a better statistical representation of storm-time radial diffusion than any single variable alone., Comment: 8 pages, 4 figures, accepted for publication in Geophysical Research Letters

Published
2015
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26. DNA Methylation as Drug Sensitivity Marker in RCC: A Systematic Review.

Author

Koudonas, Antonios, Dimitriadis, Georgios, Anastasiadis, Anastasios, and Papaioannou, Maria

Subjects
DNA methylation, RENAL cancer, CELL lines, METHYLATION, DRUG administration, METHYLGUANINE
Abstract

Patient response after treatment of renal cell cancer (RCC) with systemic agents, which include various drug categories, is generally poor and unpredictable. In this context, the ideal drug administration includes tools to predict the sensitivity of the disease to therapy. The aim of this study was to systematically summarize the reports on the predictive value of the methylation status in the systemic therapy of RCC. Only original articles reporting on the association of promoter methylation with the response of patients or cell lines to systemic agents were included in this review. We applied PRISMA recommendations to the structure and methodology of this systematic review. Our literature search concluded with 31 articles conducted on RCC cell lines and patient tissues. The majority of the studies demonstrated a methylation-dependent response to systemic agents. This correlation suggests that the methylation pattern can be used as a predictive tool in the management of RCC with various classes of systemic agents. However, although methylation biomarkers show promise for predicting response, the evidence of such correlation is still weak. More studies on the gene methylation pattern in patients under systemic therapy and its correlation with different degrees of response are needed. [ABSTRACT FROM AUTHOR]

Published
2024
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35. Review of Solar Energetic Particle Prediction Models

Author

Whitman, Kathryn, primary, Egeland, Ricky, additional, Richardson, Ian G., additional, Allison, Clayton, additional, Quinn, Philip, additional, Barzilla, Janet, additional, Kitiashvili, Irina, additional, Sadykov, Viacheslav, additional, Bain, Hazel M., additional, Dierckxsens, Mark, additional, Mays, M. Leila, additional, Tadesse, Tilaye, additional, Lee, Kerry T., additional, Semones, Edward, additional, Luhmann, Janet G., additional, Núñez, Marlon, additional, White, Stephen M., additional, Kahler, Stephen W., additional, Ling, Alan G., additional, Smart, Don F., additional, Shea, Margaret A., additional, Tenishev, Valeriy, additional, Boubrahimi, Soukaina F., additional, Aydin, Berkay, additional, Martens, Petrus, additional, Angryk, Rafal, additional, Marsh, Michael S., additional, Dalla, Silvia, additional, Crosby, Norma, additional, Schwadron, Nathan A., additional, Kozarev, Kamen, additional, Gorby, Matthew, additional, Young, Matthew A., additional, Laurenza, Monica, additional, Cliver, Edward W., additional, Alberti, Tommaso, additional, Stumpo, Mirko, additional, Benella, Simone, additional, Papaioannou, Athanasios, additional, Anastasiadis, Anastasios, additional, Sandberg, Ingmar, additional, Georgoulis, Manolis K., additional, Ji, Anli, additional, Kempton, Dustin, additional, Pandey, Chetraj, additional, Li, Gang, additional, Hu, Junxiang, additional, Zank, Gary P., additional, Lavasa, Eleni, additional, Giannopoulos, Giorgos, additional, Falconer, David, additional, Kadadi, Yash, additional, Fernandes, Ian, additional, Dayeh, Maher A., additional, Muñoz-Jaramillo, Andrés, additional, Chatterjee, Subhamoy, additional, Moreland, Kimberly D., additional, Sokolov, Igor V., additional, Roussev, Ilia I., additional, Taktakishvili, Aleksandre, additional, Effenberger, Frederic, additional, Gombosi, Tamas, additional, Huang, Zhenguang, additional, Zhao, Lulu, additional, Wijsen, Nicolas, additional, Aran, Angels, additional, Poedts, Stefaan, additional, Kouloumvakos, Athanasios, additional, Paassilta, Miikka, additional, Vainio, Rami, additional, Belov, Anatoly, additional, Eroshenko, Eugenia A., additional, Abunina, Maria A., additional, Abunin, Artem A., additional, Balch, Christopher C., additional, Malandraki, Olga, additional, Karavolos, Michalis, additional, Heber, Bernd, additional, Labrenz, Johannes, additional, Kühl, Patrick, additional, Kosovichev, Alexander G., additional, Oria, Vincent, additional, Nita, Gelu M., additional, Illarionov, Egor, additional, O’Keefe, Patrick M., additional, Jiang, Yucheng, additional, Fereira, Sheldon H., additional, Ali, Aatiya, additional, Paouris, Evangelos, additional, Aminalragia-Giamini, Sigiava, additional, Jiggens, Piers, additional, Jin, Meng, additional, Lee, Christina O., additional, Palmerio, Erika, additional, Bruno, Alessandro, additional, Kasapis, Spiridon, additional, Wang, Xiantong, additional, Chen, Yang, additional, Sanahuja, Blai, additional, Lario, David, additional, Jacobs, Carla, additional, Strauss, Du Toit, additional, Steyn, Ruhann, additional, van den Berg, Jabus, additional, Swalwell, Bill, additional, Waterfall, Charlotte, additional, Nedal, Mohamed, additional, Miteva, Rositsa, additional, Dechev, Momchil, additional, Zucca, Pietro, additional, Engell, Alec, additional, Maze, Brianna, additional, Farmer, Harold, additional, Kerber, Thuha, additional, Barnett, Ben, additional, Loomis, Jeremy, additional, Grey, Nathan, additional, Thompson, Barbara J., additional, Linker, Jon A., additional, Caplan, Ronald M., additional, Downs, Cooper, additional, Török, Tibor, additional, Lionello, Roberto, additional, Titov, Viacheslav, additional, Zhang, Ming, additional, and Hosseinzadeh, Pouya, additional

Published
2023
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39. The probabilistic solar particle event forecasting (PROSPER) model

Author

Papaioannou Athanasios, Vainio Rami, Raukunen Osku, Jiggens Piers, Aran Angels, Dierckxsens Mark, Mallios Sotirios A., Paassilta Miikka, and Anastasiadis Anastasios

Subjects
solar flares, coronal mass ejections, solar energetic particles, operational tool, validation, radiation storms, Meteorology. Climatology, QC851-999
Abstract

The Probabilistic Solar Particle Event foRecasting (PROSPER) model predicts the probability of occurrence and the expected peak flux of solar energetic particle (SEP) events. Predictions are derived for a set of integral proton energies (i.e., E > 10, > 30, and > 100 MeV) from characteristics of solar flares (longitude, magnitude), coronal mass ejections (width, speed), and combinations of both. Herein the PROSPER model methodology for deriving the SEP event forecasts is described, and the validation of the model, based on archived data, is presented for a set of case studies. The PROSPER model has been incorporated into the new operational advanced solar particle event casting system (ASPECS) tool to provide nowcasting (short term forecasting) of SEP events as part of ESA’s future SEP advanced warning system (SAWS). ASPECS also provides the capability to interrogate PROSPER for historical cases via a run-on-demand functionality.

Published
2022
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40. Bridging the Gap: Scaling Up the Sustainable Production of the Yellow Mealworm with Agricultural By-Products—Insights into Larval Growth and Body Composition.

Author

Vrontaki, Mariastela, Adamaki-Sotiraki, Christina, Rumbos, Christos I., Anastasiadis, Anastasios, and Athanassiou, Christos G.

Subjects
SUSTAINABILITY, AGRICULTURAL wastes, RICE bran, BREWER'S spent grain, BODY composition, ANIMAL feeds
Abstract

Amidst the escalating global demand for protein-rich livestock feed, there's an urgent call to explore innovative alternatives. Insects, renowned for their rich protein, lipid, and nutrient profiles, offer a sustainable solution. Integrating agricultural waste into insect diets emerges as a promising strategy to alleviate rearing costs. However, large-scale investigations into by-product valorization remain limited. Thus, our study aims to evaluate Greek agricultural by-products—brewer's spent grains, rice bran, oat and maize by-products, and animal feed mill leftovers—as potential feedstock for Tenebrio molitor larvae, an insect species that is authorized by the European Union for both livestock feed and human consumption. In this study, the larval growth and body composition were assessed in commercial trays, unveiling optimal performance with rice bran and brewer's spent grains. Conversely, larvae fed with animal feed mill leftovers and maize by-products displayed suboptimal outcomes. These findings underscore the potential efficacy of integrating locally produced agricultural by-products into T. molitor commercial production. Such an approach not only addresses the growing demand for protein-rich livestock feed but also offers a sustainable solution to agricultural waste management. In conclusion, our research contributes valuable insights towards developing economically viable insect farming. [ABSTRACT FROM AUTHOR]

Published
2024
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41. Breakage and detachment of the rigid cystoscope's distal tip: an unusual case of urological instrument malfunction.

Author

Symeonidis, Evangelos N., Symeonidis, Asterios, Anastasiadis, Anastasios, Kaltsas, Aris, Tsampoukas, Georgios, Mykoniatis, Ioannis, Memmos, Dimitrios, Toutziaris, Chrysovalantis, Dimitriadis, Fotios, Vakalopoulos, Ioannis, and Dimitriadis, Georgios

Subjects
PROSTATE cancer, BLADDER obstruction, RADICAL prostatectomy, INJURY complications, URETHRA
Abstract

Herein, we describe an unusual case of cystoscope damage during a planned laser cystolithotripsy in a 65-year-old male with a previous history of radical prostatectomy for prostate cancer and subsequent serial urethral dilations for bladder neck contracture. Upon crossing the penile urethra without exerting significant pressure, we noticed the cystoscope’s distal metallic tip detachment. Therefore, we reintroduced another 22Fr cystoscope and removed the broken part with alligator forceps. Fortunately, no urethral injury or associated complications were noticed on gently re-entering the bladder. Hence, we managed to complete the endoscopic laser cystolithotripsy shortly thereafter. Review of the relevant literature revealed three similar cases. All related to the same manufacturer. Urologists should not lose sight of the fact that such an unexpected instance may tremendously impact the procedure's success, requiring vigilance and adherence to safety protocols. [ABSTRACT FROM AUTHOR]

Published
2024
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42. Firefly: the science case for a full view of the solar sphere

Author

Harra, Louise, primary, Fletcher, Lyndsay, additional, Gizon, Laurent, additional, Solanki, Sami, additional, Romoli, Marco, additional, Harra, Louise, additional, Kusano, Kanya, additional, Hotta, Hideyuki, additional, Katsukawa, Yukio, additional, Harrison, Richard, additional, Owen, Chris, additional, Davies, Jackie, additional, Imada, Shinsuke, additional, Toriumi, Shin, additional, Tziotziou, Kostas, additional, Orozco-Suarez, David, additional, Verscharen, Daniele, additional, Papaioannou, Athanasios, additional, Milligan, Ryan, additional, Tsiropoula, Georgia, additional, Hara, Hiroshisa, additional, Shimizu, Toshifumi, additional, Krucker, Säm, additional, Mackay, Duncan, additional, Berghmans, David, additional, Dominique, Marie, additional, Dolla, Laurent, additional, Shestov, Sergei, additional, Daglis, Ioannis, additional, Balasis, George, additional, Nindos, Alexander, additional, Moraitis, Kostis, additional, Gontikakis, Costis, additional, Matthews, Sarah, additional, Moortel, Ineke De, additional, Moussas, Xenophon, additional, Iniesta, Jose Carlos del Toro, additional, Mathioudakis, Mihalis, additional, Rodriguez-Pacheco, Javier, additional, Spadaro, Daniele, additional, Gallagher, Peter, additional, Andretta, Vincenzo, additional, Fazakerley, Andrew, additional, Auchère, Frederic, additional, Fineschi, Silvano, additional, Telloni, Daniele, additional, Wimmer-Schweingruber, Robert, additional, Kleint, Lucia, additional, Peter, Hardi, additional, Krivova, Natalie, additional, Chitta, Lakshmi Pradeeep, additional, Barczynski, Krzysztof, additional, Finsterle, Wolfgang, additional, Rouillard, Alexis, additional, McLaughlin, James, additional, Raouafi, Nour E., additional, Verscharen, Daniel, additional, Dalla, Silvia, additional, and Anastasiadis, Anastasios, additional

Published
2023
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43. Firefly: The Case for a Holistic Understanding of the Global Structure and Dynamics of the Sun and the Heliosphere

Author

Raouafi, Nour E., primary, Hoeksema, J. Todd, additional, Newmark, Jeffrey S., additional, Gibson, Sarah, additional, Berger, Thomas E., additional, Upton, Lisa A., additional, Vourlidas, Angelos, additional, Hassler, Donald M., additional, Kinnison, James, additional, Ho, George C., additional, Mason, Glenn M., additional, Vievering, Juliana T., additional, Viall, Nicholeen M., additional, Szabo, Adam, additional, Casti, Marta, additional, Case, Anthony W., additional, Lepri, Susan T., additional, Velli, Marco, additional, Georgoulis, Manolis K., additional, Bourouaine, Sofiane, additional, Jagarlamudi, Vamsee K., additional, Laming, John M., additional, Mason, James P., additional, Harra, Louise, additional, Madjarska, Maria, additional, Chitta, Lakshmi Pradeep, additional, Duran, J. Sebastian Castellanos, additional, Korpi-Lagg, Andreas, additional, Badman, Samuel, additional, Chifu, Iulia, additional, Lario, David, additional, Wing, Simon, additional, Bale, Stuart, additional, Paouris, Evangelos, additional, Narayanamurthy, Smitha, additional, Sinjan, Jonas, additional, Bernasconi, Pietro, additional, Krivova, Natalie, additional, Gizon, Laurent, additional, Leamon, Robert J., additional, Gosain, Sanjay, additional, Kazachenko, Maria, additional, Petrie, Gordon, additional, Pillet, Valentin Martinez, additional, Jain, Kiran, additional, Luhmann, Janet, additional, Bertello, Luca, additional, Toriumi, Shin, additional, Jiang, Chen, additional, Vasko, Ivan, additional, Harvey, John W., additional, Schad, Thomas A., additional, Jebaraj, Immanuel C., additional, Scherrer, Philip, additional, Hofmeister, Stefan, additional, Tiwari, Sanjiv, additional, Wang, Haimin, additional, Roth, Markus, additional, Panesar, Navdeep, additional, Sekii, Takashi, additional, Magyar, Norbert, additional, Guglielmino, Salvo L., additional, Parenti, Susanna, additional, Tremblay, Benoit, additional, Tziotziou, Kostas, additional, Toma, Giuliana de, additional, Chen, Bin, additional, Katsukawa, Yukio, additional, Pontieu, Bart De, additional, Cheng, Xin, additional, Cheung, Mark, additional, Kosovichev, Alexander, additional, Jiang, Jie, additional, Schunker, Hannah, additional, Kawabata, Yusuke, additional, Oba, Takayoshi, additional, Cameron, Robert, additional, Mathew, Shibu K., additional, Rodriguez, Jaime de la Cruz, additional, Kusano, Kanya, additional, Temmer, Manuela, additional, Andretta, Vincenzo, additional, Sven, Wedemeyer, additional, Samara, Evangelia, additional, Heinemann, Stephan G., additional, Warmuth, Alexander, additional, Jafarzadeh, Shahin, additional, Mackay, Duncan H., additional, Fludra, Andrzej, additional, Rubio, Luis Bellot, additional, Suárez, David Orozco, additional, Chen, Thomas Y., additional, Kontogiannis, Ioannis, additional, Yardley, Stephanie, additional, Veronig, Astrid, additional, Joshi, Jayant, additional, Spadaro, Daniele, additional, Kubo, Masahito, additional, Bose, Souvik, additional, González, Nazaret Bello, additional, Solanki, Sami, additional, Denker, Carsten, additional, Verma, Meetu, additional, Vocks, Christian, additional, Borrero, Juan Manuel, additional, Mathews, Nathaniel H., additional, Cury, Shannon, additional, Sasso, Clementina, additional, Stenborg, Guillermo, additional, Tibebu, Getachew, additional, Battams, Karl, additional, Wijsen, Nicolas, additional, Bruno, Alessandro, additional, Peter, Hardi, additional, I., Mason Emily, additional, M., Caplan Ronald, additional, Martinez-Sykora, Juan, additional, Seaton, Daniel, additional, Airapetian, Vladimir, additional, Jian, Lan, additional, Thompson, William T., additional, Ofman, Leon, additional, Wallace, Samantha, additional, Kucera, Therese, additional, Desai, Ravindra, additional, Richardson, Ian, additional, Burkepile, Joan, additional, Cranmer, Steven, additional, Strauss, R. Du Toit, additional, Murabito, Mariarita, additional, Alfred, De Wijn, additional, Xie, Hong, additional, Rempel, Matthias, additional, Webber, Shea Hess, additional, Reeves, Katharine K., additional, Hurlburt, Neal, additional, Berrilli, Francesco, additional, DeLuca, Edward, additional, Egeland, Ricky, additional, Ko, Yuan-Kuen, additional, Kee, Nathaniel Dylan, additional, Mahajan, Sushant S., additional, Craig, DeForest, additional, Wood, Brian E., additional, Chris, Chaston, additional, Nigro, Giuseppina, additional, Shaik, Shaheda Begum, additional, Gosic, Milan, additional, Shimizu, Toshifumi, additional, Zuccarello, Francesca, additional, Nitta, Nariaki, additional, Chatzistergos, Theodosios, additional, Fan, Yuhong, additional, Zhang, Jie, additional, Fehlmann, Andre, additional, Palmerio, Erika, additional, Ishikawa, Ryohtaroh T., additional, Danilovic, Sanja, additional, Skan, Moa, additional, Froment, Clara, additional, Baso, Carlos José Díaz, additional, Liang, Zhi-Chao, additional, Wit, Thierry Dudok de, additional, Barczynski, Krzysztof, additional, Johnston, Craig, additional, Pariat, Etienne, additional, Hadid, Lina, additional, Aulanier, Guillaume, additional, Brun, Allan Sacha, additional, Athanasios, Kouloumvakos, additional, Cauzzi, Gianna, additional, Dredger, Pauline, additional, French, Ryan, additional, Christian, Damian, additional, Linton, Mark, additional, Ireland, Jack, additional, Tarr, Lucas, additional, Strugarek, Antoine, additional, Uritsky, Vadim, additional, DeRosa, Marc, additional, Kretzschmar, Matthieu, additional, García, Rafael A., additional, Monteiro, Mario J. P. F. G., additional, Mathur, Savita, additional, Breton, Sylvain N., additional, Pinto, Rui F., additional, Oliveros, Juan Carlos Martinez, additional, Loper, Robert, additional, Auchère, Frédéric, additional, Wang, Tongjiang, additional, Reginald, Nelson, additional, Cunha, Margarida S., additional, Teriaca, Luca, additional, Chintzoglou, Georgios, additional, Lynch, Benjamin J., additional, Linker, Jon, additional, Beck, Paul, additional, Shannon, Jackson, additional, Clare, Benjamin, additional, Krupiarz, Christopher, additional, Whiting, Ian D., additional, Byerly, Adam, additional, Bushman, Stewart, additional, Carrelli, David, additional, Kijewski, Seth, additional, Englander, Jacob, additional, Mizes, Adam, additional, Porter, Jamie, additional, O’Neill, Michael, additional, Chattopadhyay, Debarati, additional, Albers, Joshua, additional, Rast, Mark, additional, Ermolli, Ilaria, additional, Tzeng, Nigel, additional, Hudson, James F., additional, Giunta, Alessandra, additional, Buchlin, Éric, additional, Bommier, Véronique, additional, Duncan, Nicole, additional, Janvier, Miho, additional, Strecker, Hanna, additional, Siu, Azaymi, additional, Perri, Barbara, additional, Maksimovic, Milan, additional, Vilmer, Nicole, additional, Toledo-Redondo, Sergio, additional, Kuckein, Christoph, additional, Alberti, Tommaso, additional, Antolin, Patrick, additional, Cuadrado, Regina Aznar, additional, Berghmans, David, additional, Brigitte, Schmieder, additional, Bucik, Radoslav, additional, Calchetti, Daniele, additional, Caspi, Amir, additional, Cohen, Christina, additional, Corbard, Thierry, additional, Cremades, Hebe, additional, Cummings, Alan, additional, Dhakal, Suman, additional, Dolla, Laurent, additional, Dominique, Marie, additional, Emslie, Gordon, additional, Ferrente, Fabiana, additional, Finley, Adam J., additional, Fletcher, Lyndsay, additional, Fraschetti, Federico, additional, Gafeira, Ricardo, additional, Gissot, Samuel, additional, Hegde, Dinesha, additional, Hu, Qiang, additional, Innocenti, Maria Elena, additional, Jin, Meng, additional, Klein, Kristopher, additional, Kumar, Pankaj, additional, Lacatus, Daniela, additional, Liewer, Paulett, additional, Magdalenic, Jasmina, additional, Mandal, Sudip, additional, Mandrini, Cristina H., additional, Mierla, Marilena, additional, Miralles, Mari Paz, additional, Moore, Ron, additional, Neville, Jonathan, additional, Niembro, Tatiana, additional, Nikou, Eleni, additional, Nindos, Alexander, additional, Papaioannou, Athanasios, additional, Rajaguru, S. Paul, additional, Reville, Victor, additional, Rochus, Pierre, additional, Rodriguez, Luciano, additional, Romoli, Marco, additional, Shestov, Sergei, additional, Shi, Chen, additional, Sorriso-Valvo, Luca, additional, St. Cyr, O. C., additional, Sterling, Alphohse, additional, Stevens, Michael L., additional, Susino, Roberto, additional, Swisdak, Marc, additional, Thompson, Barbara J., additional, Valliappan, Senthamizh Pavai, additional, Verbeeck, Francis, additional, Bothmer, Volker, additional, Xudong, Sun, additional, Zhukov, Andrei, additional, Katsiyannis, Thanassis, additional, Owen, Christopher, additional, Karna, Nishu, additional, Janssens, Jan, additional, Khomenko, Elena, additional, Gary, Dale, additional, Bandyopadhyay, Riddhi, additional, Chhiber, Rohit, additional, Tenerani, Anna, additional, Rouillard, Alexis, additional, Patsourakos, Spiros, additional, Anastasiadis, Anastasios, additional, Bocchialini, Karine, additional, Moraitis, Kostas, additional, Rivera, Yeimy, additional, Drake, James, additional, Baudin, Frédéric, additional, Chandran, Benjamin, additional, Dayeh, Maher, additional, Reardon, Kevin, additional, Cairns, Iver, additional, Bizien, Nina, additional, Wexler, David, additional, Bahauddin, Shah, additional, Rodriguez-Pacheco, Javier, additional, Yu, Sijie, additional, Lee, Jeongwoo, additional, Gontikakis, Costis, additional, Koukras, Alexandros, additional, Contel, Olivier Le, additional, Pezzi, Oreste, additional, Kintziger, Christian, additional, Boumier, Patrick, additional, Balasis, Georgios, additional, Dikpati, Mausumi, additional, Pesnell, W. Dean, additional, Chai, Yi, additional, Nandy, Dibyendu, additional, Charles, Arge, additional, Corti, Claudio, additional, Zhao, Lulu, additional, Matthaeus, William H., additional, Gilly, Chris R., additional, Erlandson, Robert E., additional, Derouich, Moncef, additional, Zhao, Lingling, additional, Poedts, Stefaan, additional, Vieira, Luis, additional, Adhikari, Laxman, additional, Buitrago-Casas, Juan Camilo, additional, Huang, Jia, additional, Moestl, Christian, additional, Liu, Mingzhe, additional, Oloketuyi, Jacob, additional, Zhuang, Bin, additional, Rodríguez-García, Laura, additional, Perez, Jean Carlos, additional, Xu, Zigong, additional, Kooi, Jason, additional, Woodham, Lloyd D., additional, Tripathi, Durgesh, additional, Young, Peter, additional, López-Portela, Cynthia, additional, Cuesta, Manuel Enrique, additional, and Wilson, Lynn, additional

Published
2023
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44. Overview of current pharmacotherapeutic options in benign prostatic hyperplasia

Author

Koudonas, Antonios, primary, Anastasiadis, Anastasios, additional, Tsiakaras, Stavros, additional, Langas, Georgios, additional, Savvides, Eliophotos, additional, Mykoniatis, Ioannis, additional, Memmos, Dimitrios, additional, Baniotis, Panagiotis, additional, Vakalopoulos, Ioannis, additional, de la Rosette, Jean, additional, and Dimitriadis, Georgios, additional

Published
2023
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45. Predicting the Impact of Solar Energetic Particles - the ADVISOR Research Project

Author

Papaioannou, Athanasios, Anastasiadis, Anastasios, Vasalos, George, Milas, Nick, Mays, M. Leila, Jones, Joycelyn, Quinn, Phil, Semones, Edward, Whitman, Kathryn, and Barzilla, Janet

Abstract

A system that is in place to predict the impact of Solar Energetic Particles (SEPs) on the radiation environment is of paramount importance for the upcoming critical space exploration missions. In the coming years, astronauts will be sent to the Moon and Mars, expanding the frontiers of current knowledge. Therefore, reliable prediction systems that will deliver timely warnings on the potential of a solar eruptive event to give rise to an upcoming SEP are much needed. Currently, thorough evaluation, understanding, validation, expansion and optimization of such available predicting systems are taking place. The ADVISOR (OptimizAtion, DeliVery & Installation of the ASPECS tOol for Space WeatheR research within ISEP) project [https://members.noa.gr/atpapaio/advisor/] builds upon the ASPECS (Advanced Solar Particle Event Casting System) tool [http://phobos-srv.space.noa.gr/], a 3-tier system combining the forecasting of flares, the statistical forecast of events on the basis of flare and CME characteristics and physics and analytical modeling for predicting particle flux profiles, leading to the complete time profile of SEPs at respective energies of interest. Taking into account the initial efforts that resulted to the integration of the ASPECS’s outputs to the NASA Community Coordinated Modeling Center (CCMC) SEP Scoreboard [https://ccmc.gsfc.nasa.gov/scoreboards/sep/], with the involvement of NASA SRAG (Space Radiation Analysis Group) and the Moon to Mars (M2M) Space Weather Analysis Office, ADVISOR improves and stabilizes the functionalities and outputs offered by ASPECS. In this work, all technical and scientific refinements and updates are presented., {"references":["Papaioannou, Athanasios et al. (2022). The Probabilistic Solar Particle Event foRecasting (PROSPER) Model. arXiv:2205.07325"]}

Published
2023
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49. Review of Solar Energetic Particle Models

Author

Whitman, Kathryn, Egeland, Ricky, Richardson, Ian G, Allison, Clayton, Quinn, Philip, Barzilla, Janet, Kitiashvili, Irina, Sadykov, Viacheslav, Bain, Hazel M, Dierckxsens, Mark, Mays, M Leila, Tadesse, Tilaye, Lee, Kerry T, Semones, Edward, Luhmann, Janet G, Nunez, Marlon, White, Stephen M, Kahler, Stephen W, Ling, Alan G, Smart, Don F, Shea, Margaret A, Tenishev, Valeriy, Soukaina F, Boubrahimi, Aydin, Berkay, Martens, Petrus, Angryk, Rafal, Marsh, Michael S, Dalla, Silvia, Crosby, Norma, Schwadron, Nathan A, Kozarev, Kamen, Gorby, Matthew, Young, Matthew A, Laurenza, Monica, Cliver, Edward W, Alberti, Tommaso, Stumpo, Mirko, Benella, Simone, Papaioannou, Athanasios, Anastasiadis, Anastasios, Sandberg, Ingmar, Georgoulis, Manolis K, Ji, Anli, Kempton, Dustin, Pandey, Chetraj, Li, Gang, Hu, Junxiang, Zank, Gary P, Lavasa, Eleni, Giannopoulos, Giorgos, Falconer, David, Kadadi, Yash, Fernandes, Ian, Dayeh, Maher A, Munoz-Jaramillo, Andres, Chatterjee, Subhamoy, Moreland, Kimberly D, Sokolov, Igor V, Roussec, Ilia I, Taktakishvili, Aleksandre, Effenberger, Frederic, Gombosi, Tamas, Huang, Zhenguang, Zhao, Lulu, Wijsen, Nicolas, Aran, Angels, Poedts, Stefaan, Kouloumvakos, Athanasios, Paassilita, Miikka, Vainio, Rami, Belov, Anatoly, Eroshenko, Eugenia A, Abunina, Maria A, Abunin, Artem A, Balch, Christopher C, Malandraki, Olga, Karavolos, Michalis, Herber, Bernd, Labrenz, Johannes, Kühl, Patrick, Kosovichev, Alexander G, Oria, Vincent, Nita, Gelu M, Illarionov, Egor, O'Keefe, PAtrick M, Jiang, Yucheng, Fereira, Sheldon H, Ali, Aatiya, Paouris, Evangelos, Aminalfragia-Giamini, Sigiava, Jiggens, Piers, Jin, Meng, Lee, Christina O, Palmerio, Erika, Bruno, Alessandro, Kasapis, Spiridon, Wang, Xiantong, Cheng, Yang, Sanahuja, Blai, Lario, David, Jacobs, Carla, Strauss, Du Toit, Steyn, Ruhann, den Berg van, Jabus, Swalwell, Bill, Waterfall, Charlotte, Nedal, Mohamed, Miteva, Rositsa, Dechev, Momchil, Zucca, Pietro, Engell, Alec, Maze, Brianna, Farmer, Harold, Kerber, Thuha, Barnett, Ben, Loomis, Jeremy, Grey, Nathan, Thompson, Barbara J, Linker, Jon A, Caplan, Ronald M, Downs, Cooper, Török, Tibor, Linello, Roberto, Titov, Viacheslav, Zhang, Ming, Hosseinzadeh, Pouya, Whitman, Kathryn, Egeland, Ricky, Richardson, Ian G, Allison, Clayton, Quinn, Philip, Barzilla, Janet, Kitiashvili, Irina, Sadykov, Viacheslav, Bain, Hazel M, Dierckxsens, Mark, Mays, M Leila, Tadesse, Tilaye, Lee, Kerry T, Semones, Edward, Luhmann, Janet G, Nunez, Marlon, White, Stephen M, Kahler, Stephen W, Ling, Alan G, Smart, Don F, Shea, Margaret A, Tenishev, Valeriy, Soukaina F, Boubrahimi, Aydin, Berkay, Martens, Petrus, Angryk, Rafal, Marsh, Michael S, Dalla, Silvia, Crosby, Norma, Schwadron, Nathan A, Kozarev, Kamen, Gorby, Matthew, Young, Matthew A, Laurenza, Monica, Cliver, Edward W, Alberti, Tommaso, Stumpo, Mirko, Benella, Simone, Papaioannou, Athanasios, Anastasiadis, Anastasios, Sandberg, Ingmar, Georgoulis, Manolis K, Ji, Anli, Kempton, Dustin, Pandey, Chetraj, Li, Gang, Hu, Junxiang, Zank, Gary P, Lavasa, Eleni, Giannopoulos, Giorgos, Falconer, David, Kadadi, Yash, Fernandes, Ian, Dayeh, Maher A, Munoz-Jaramillo, Andres, Chatterjee, Subhamoy, Moreland, Kimberly D, Sokolov, Igor V, Roussec, Ilia I, Taktakishvili, Aleksandre, Effenberger, Frederic, Gombosi, Tamas, Huang, Zhenguang, Zhao, Lulu, Wijsen, Nicolas, Aran, Angels, Poedts, Stefaan, Kouloumvakos, Athanasios, Paassilita, Miikka, Vainio, Rami, Belov, Anatoly, Eroshenko, Eugenia A, Abunina, Maria A, Abunin, Artem A, Balch, Christopher C, Malandraki, Olga, Karavolos, Michalis, Herber, Bernd, Labrenz, Johannes, Kühl, Patrick, Kosovichev, Alexander G, Oria, Vincent, Nita, Gelu M, Illarionov, Egor, O'Keefe, PAtrick M, Jiang, Yucheng, Fereira, Sheldon H, Ali, Aatiya, Paouris, Evangelos, Aminalfragia-Giamini, Sigiava, Jiggens, Piers, Jin, Meng, Lee, Christina O, Palmerio, Erika, Bruno, Alessandro, Kasapis, Spiridon, Wang, Xiantong, Cheng, Yang, Sanahuja, Blai, Lario, David, Jacobs, Carla, Strauss, Du Toit, Steyn, Ruhann, den Berg van, Jabus, Swalwell, Bill, Waterfall, Charlotte, Nedal, Mohamed, Miteva, Rositsa, Dechev, Momchil, Zucca, Pietro, Engell, Alec, Maze, Brianna, Farmer, Harold, Kerber, Thuha, Barnett, Ben, Loomis, Jeremy, Grey, Nathan, Thompson, Barbara J, Linker, Jon A, Caplan, Ronald M, Downs, Cooper, Török, Tibor, Linello, Roberto, Titov, Viacheslav, Zhang, Ming, and Hosseinzadeh, Pouya

Abstract

Solar Energetic Particles (SEP) events are interesting from a scientific perspective as they are the product of a broad set of physical processes from the corona out through the extent of the heliosphere, and provide insight into processes of particle acceleration and transport that are widely applicable in astrophysics. From the operations perspective, SEP events pose a radiation hazard for aviation, electronics in space, and human space exploration, in particular for missions outside of the Earth’s protective magnetosphere including to the Moon and Mars. Thus, it is critical to imific understanding of SEP events and use this understanding to develop and improve SEP forecasting capabilities to support operations. Many SEP models exist or are in development using a wide variety of approaches and with differing goals. These include computationally intensive physics-based models, fast and light empirical models, machine learning-based models, and mixed-model approaches. The aim of this paper is to summarize all of the SEP models currently developed in the scientific community, including a description of model approach, inputs and outputs, free parameters, and any published validations or comparisons with data.

Published
2023

50. The effect of standard percutaneous nephrolithotomy, miniaturized percutaneous nephrolithotomy and retrograde intrarenal surgery on biomarkers of renal injury: a randomized clinical trial

Author

Memmos, Dimitrios, primary, Sarafidis, Pantelis, additional, Alexandrou, Maria Eleni, additional, Theodorakopoulou, Marieta, additional, Anastasiadis, Anastasios, additional, Mykoniatis, Ioannis, additional, Dimitriadis, Georgios, additional, and Hatzichristou, Dimitrios, additional

Published
2023
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