48 results on '"Habbal, Shadia"'
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2. The Color and Brightness of the F-corona Inferred from the 2019 July 2 Total Solar Eclipse
3. Coronal Magnetic Field Topology from Total Solar Eclipse Observations
4. CME-induced Thermodynamic Changes in the Corona as Inferred from Fe xi and Fe xiv Emission Observations during the 2017 August 21 Total Solar Eclipse
5. Exploring the fine structure at the limb in coronal holes
6. The First Empirical Determination of the Fe10+ and Fe13+ Freeze-in Distances in the Solar Corona
7. Tethered Prominence-CME Systems Captured during the 2012 November 13 and 2013 November 3 Total Solar Eclipses
8. Dynamics of Large-scale Coronal Structures as Imaged during the 2012 and 2013 Total Solar Eclipses
9. First Detection of Prominence Material Embedded within a 2 × 10 6 K CME Front Streaming away at 100–1500 km s −1 in the Solar Corona
10. EXPLORING THE PROMINENCE-CORONA CONNECTION AND ITS EXPANSION INTO THE OUTER CORONA USING TOTAL SOLAR ECLIPSE OBSERVATIONS
11. DISCOVERY OF A NEW CLASS OF CORONAL STRUCTURES IN WHITE LIGHT ECLIPSE IMAGES
12. IMAGING COMET ISON C/2012 S1 IN THE INNER CORONA AT PERIHELION
13. THE PERIOD RATIO FOR STANDING KINK AND SAUSAGE MODES IN SOLAR STRUCTURES WITH SIPHON FLOW. I. MAGNETIZED SLABS
14. AUTOMATICALLY DETECTING AND TRACKING CORONAL MASS EJECTIONS. I. SEPARATION OF DYNAMIC AND QUIESCENT COMPONENTS IN CORONAGRAPH IMAGES
15. AUTOMATIC DETECTION AND TRACKING OF CORONAL MASS EJECTIONS. II. MULTISCALE FILTERING OF CORONAGRAPH IMAGES
16. ENHANCING CORONAL STRUCTURES WITH THE FOURIER NORMALIZING-RADIAL-GRADED FILTER
17. OBSERVATION OF HIGH-SPEED OUTFLOW ON PLUME-LIKE STRUCTURES OF THE QUIET SUN AND CORONAL HOLES WITHSOLAR DYNAMICS OBSERVATORY/ATMOSPHERIC IMAGING ASSEMBLY
18. THERMODYNAMICS OF THE SOLAR CORONA AND EVOLUTION OF THE SOLAR MAGNETIC FIELD AS INFERRED FROM THE TOTAL SOLAR ECLIPSE OBSERVATIONS OF 2010 JULY 11
19. ON THE CONSTANCY OF THE ELECTRON TEMPERATURE IN THE EXPANDING CORONA THROUGHOUT SOLAR CYCLE 23
20. A METHOD FOR SEPARATING CORONAL MASS EJECTIONS FROM THE QUIESCENT CORONA
21. OBSERVATIONAL ASPECTS OF THE THREE-DIMENSIONAL CORONAL STRUCTURE OVER A SOLAR ACTIVITY CYCLE
22. MAPPING THE STRUCTURE OF THE CORONA USING FOURIER BACKPROJECTION TOMOGRAPHY
23. Impact of Active Regions on Coronal Hole Outflows
24. Erratum: “Localized Enhancements of Fe+10Density in the Corona as Observed in Fexi789.2 nm during the 2006 March 29 Total Solar Eclipse” (ApJ, 663, 598 [2007])
25. Localized Enhancements of Fe+10Density in the Corona as Observed in Fexi789.2 nm during the 2006 March 29 Total Solar Eclipse
26. Angular Momentum Transport and Proton–Alpha‐Particle Differential Streaming in the Solar Wind
27. Origin and Acceleration of the Slow Solar Wind
28. Crystalline Si Nanoparticles as Carriers of the Blue Luminescence in the Red Rectangle Nebula
29. Role of Closed Magnetic Fields in Solar Wind Flow
30. Coronal Loops Heated by Turbulence-driven Alfvn Waves
31. On the Detection of the Signature of Silicon Nanoparticle Dust Grains in Coronal Holes
32. On the Predominance of the Radial Component of the Magnetic Field in the Solar Corona
33. Connecting the Sun and the Solar Wind: Comparison of the Latitudinal Profiles of Coronal and [ITAL]Ulysses[/ITAL] Measurements of the Fast Wind
34. Observed Associations between the Solar Interior, Corona, and Solar Wind
35. Extension of the Polar Coronal Hole Boundary into Interplanetary space
36. Plasma Properties in Coronal Holes Derived from Measurements of Minor Ion Spectral Lines and Polarized White Light Intensity
37. Imprint of the Sun on the Solar Wind
38. The Effect of Temperature Anisotropy on Observations of Doppler Dimming and Pumping in the Inner Corona
39. Finest Filamentary Structures of the Corona in the Slow and Fast Solar Wind
40. The Effects on Mass Flows on the Dissipation of Alfven Waves in the Upper Layers of the Solar Atmosphere
41. Dynamical structure of extreme ultraviolet macrospicules
42. On the derivation of empirical limits on the helium abundance in coronal holes below 1.5 solar radius
43. The connection between coronal bright points and the variability of the quiet-sun extreme-ultraviolet emission
44. First observations of microspicules at 4.8 GHz at the solar limb in polar coronal holes
45. High-resolution studies of the structure of the solar atmosphere using a new imaging algorithm
46. A comparison between bright points in a coronal hole and a quiet-sun region
47. Synthesis mapping of a solar type I storm simultaneously at 90 and 20 centimeters with the VLA
48. Simultaneous observations of 20 centimeter bright points and He I 10830 A dark points in the quiet sun
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