79 results on '"McIntosh, Scott"'
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2. Information-theoretic Analysis of Longitude Distribution of Photospheric Magnetic Fields from MDI/HMI Synoptic Maps: Evidence for Rossby Waves
3. Magnetohydrodynamic Instabilities of Double Magnetic Bands in a Shallow-water Tachocline Model. I. Cross-equatorial Interactions of Bands
4. Simulating Solar Near-surface Rossby Waves by Inverse Cascade from Supergranule Energy
5. Tracking Movement of Long-lived Equatorial Coronal Holes from Analysis of Long-term McIntosh Archive Data
6. Probing the Physics of the Solar Atmosphere with the Multi-slit Solar Explorer (MUSE). I. Coronal Heating
7. Dynamical Splitting of Spot-producing Magnetic Rings in a Nonlinear Shallow-water Model
8. Deciphering the Deep Origin of Active Regions via Analysis of Magnetograms
9. Deciphering Solar Magnetic Activity. I. On the Relationship Between the Sunspot Cycle and the Evolution of Small Magnetic Features
10. Investigating the Chromospheric Footpoints of the Solar Wind
11. Prediction of the In Situ Coronal Mass Ejection Rate for Solar Cycle 25: Implications for Parker Solar Probe In Situ Observations
12. Physics of Magnetohydrodynamic Rossby Waves in the Sun
13. The Drivers of Active Region Outflows into the Slow Solar Wind
14. Persistent Doppler Shift Oscillations Observed with HINODE-EIS in the Solar Corona: Spectroscopic Signatures of Alfvenic Waves and Recurring Upflows
15. Signature of Extended Solar Cycles as Detected from Ca ii K Synoptic Maps of Kodaikanal and Mount Wilson Observatory
16. Phase Speed of Magnetized Rossby Waves that Cause Solar Seasons
17. Erratum: “On the Magnetic and Energy Characteristics of Homologous Jets From an Emerging Flux” (2016, ApJ, 833, 150)
18. Role of Interaction between Magnetic Rossby Waves and Tachocline Differential Rotation in Producing Solar Seasons
19. North–South Asymmetry in Rieger-type Periodicity during Solar Cycles 19–23
20. ON THE MAGNETIC AND ENERGY CHARACTERISTICS OF RECURRENT HOMOLOGOUS JETS FROM AN EMERGING FLUX
21. ON THE OBSERVATION AND SIMULATION OF SOLAR CORONAL TWIN JETS
22. ON THE PARALLEL AND PERPENDICULAR PROPAGATING MOTIONS VISIBLE IN POLAR PLUMES: AN INCUBATOR FOR (FAST) SOLAR WIND ACCELERATION?
23. STATISTICAL EVIDENCE FOR THE EXISTENCE OF ALFVÉNIC TURBULENCE IN SOLAR CORONAL LOOPS
24. ON MAGNETIC ACTIVITY BAND OVERLAP, INTERACTION, AND THE FORMATION OF COMPLEX SOLAR ACTIVE REGIONS
25. ROTATING SOLAR JETS IN SIMULATIONS OF FLUX EMERGENCE WITH THERMAL CONDUCTION
26. IDENTIFYING POTENTIAL MARKERS OF THE SUN'S GIANT CONVECTIVE SCALE
27. A DETAILED COMPARISON BETWEEN THE OBSERVED AND SYNTHESIZED PROPERTIES OF A SIMULATED TYPE II SPICULE
28. HEMISPHERIC ASYMMETRIES OF SOLAR PHOTOSPHERIC MAGNETISM: RADIATIVE, PARTICULATE, AND HELIOSPHERIC IMPACTS
29. ESTIMATING THE “DARK” ENERGY CONTENT OF THE SOLAR CORONA
30. PERSISTENT DOPPLER SHIFT OSCILLATIONS OBSERVED WITHHINODE/EIS IN THE SOLAR CORONA: SPECTROSCOPIC SIGNATURES OF ALFVÉNIC WAVES AND RECURRING UPFLOWS
31. ON THE DOPPLER VELOCITY OF EMISSION LINE PROFILES FORMED IN THE “CORONAL CONTRAFLOW” THAT IS THE CHROMOSPHERE-CORONA MASS CYCLE
32. WHAT CAN WE LEARN ABOUT SOLAR CORONAL MASS EJECTIONS, CORONAL DIMMINGS, AND EXTREME-ULTRAVIOLET JETS THROUGH SPECTROSCOPIC OBSERVATIONS?
33. THE CONNECTION OF TYPE II SPICULES TO THE CORONA
34. SOLAR CYCLE VARIATIONS IN THE ELEMENTAL ABUNDANCE OF HELIUM AND FRACTIONATION OF IRON IN THE FAST SOLAR WIND: INDICATORS OF AN EVOLVING ENERGETIC RELEASE OF MASS FROM THE LOWER SOLAR ATMOSPHERE
35. TWO COMPONENTS OF THE SOLAR CORONAL EMISSION REVEALED BY EXTREME-ULTRAVIOLET SPECTROSCOPIC OBSERVATIONS
36. OBSERVATION OF HIGH-SPEED OUTFLOW ON PLUME-LIKE STRUCTURES OF THE QUIET SUN AND CORONAL HOLES WITHSOLAR DYNAMICS OBSERVATORY/ATMOSPHERIC IMAGING ASSEMBLY
37. WHAT DO SPECTRAL LINE PROFILE ASYMMETRIES TELL US ABOUT THE SOLAR ATMOSPHERE?
38. OBSERVING EVOLUTION IN THE SUPERGRANULAR NETWORK LENGTH SCALE DURING PERIODS OF LOW SOLAR ACTIVITY
39. THE SPECTROSCOPIC SIGNATURE OF QUASI-PERIODIC UPFLOWS IN ACTIVE REGION TIMESERIES
40. THE SPECTROSCOPIC FOOTPRINT OF THE FAST SOLAR WIND
41. QUASI-PERIODIC PROPAGATING SIGNALS IN THE SOLAR CORONA: THE SIGNATURE OF MAGNETOACOUSTIC WAVES OR HIGH-VELOCITY UPFLOWS?
42. HIGH-SPEED TRANSITION REGION AND CORONAL UPFLOWS IN THE QUIET SUN
43. OBSERVING EPISODIC CORONAL HEATING EVENTS ROOTED IN CHROMOSPHERIC ACTIVITY
44. ESTIMATING THE CHROMOSPHERIC ABSORPTION OF TRANSITION REGION MOSS EMISSION
45. OBSERVING THE ROOTS OF SOLAR CORONAL HEATING—IN THE CHROMOSPHERE
46. TIME-DISTANCE SEISMOLOGY OF THE SOLAR CORONA WITH CoMP
47. HOW THE SOLAR WIND TIES TO ITS PHOTOSPHERIC ORIGINS
48. THE INCONVENIENT TRUTH ABOUT CORONAL DIMMINGS
49. Impact of Active Regions on Coronal Hole Outflows
50. The Energy Flux of Internal Gravity Waves in the Lower Solar Atmosphere
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