These tools will no longer be maintained as of December 31, 2024. Archived website can be found here. PubMed4Hh GitHub repository can be found here. Contact NLM Customer Service if you have questions.
135 related articles for article (PubMed ID: 31949076)
41. Heating and Cooling of Coronal Loops with Turbulent Suppression of Parallel Heat Conduction. Bian N; Emslie AG; Horne D; Kontar EP Astrophys J; 2018 Jan; 852(No 2):. PubMed ID: 29430026 [TBL] [Abstract][Full Text] [Related]
42. Coronal magnetohydrodynamic waves and oscillations: observations and quests. Aschwanden MJ Philos Trans A Math Phys Eng Sci; 2006 Feb; 364(1839):417-32; discussion 432. PubMed ID: 16414888 [TBL] [Abstract][Full Text] [Related]
43. The Instruments and Capabilities of the Moore CS; Caspi A; Woods TN; Chamberlin PC; Dennis BR; Jones AR; Mason JP; Schwartz RA; Tolbert AK Sol Phys; 2018; 293(2):21. PubMed ID: 31258201 [TBL] [Abstract][Full Text] [Related]
45. Transient rotation of photospheric vector magnetic fields associated with a solar flare. Xu Y; Cao W; Ahn K; Jing J; Liu C; Chae J; Huang N; Deng N; Gary DE; Wang H Nat Commun; 2018 Jan; 9(1):46. PubMed ID: 29298973 [TBL] [Abstract][Full Text] [Related]
47. Chromospheric alfvenic waves strong enough to power the solar wind. De Pontieu B; McIntosh SW; Carlsson M; Hansteen VH; Tarbell TD; Schrijver CJ; Title AM; Shine RA; Tsuneta S; Katsukawa Y; Ichimoto K; Suematsu Y; Shimizu T; Nagata S Science; 2007 Dec; 318(5856):1574-7. PubMed ID: 18063784 [TBL] [Abstract][Full Text] [Related]
48. Self-similar signature of the active solar corona within the inertial range of solar-wind turbulence. Kiyani K; Chapman SC; Hnat B; Nicol RM Phys Rev Lett; 2007 May; 98(21):211101. PubMed ID: 17677760 [TBL] [Abstract][Full Text] [Related]
49. Solar Energetic Particle Forecasting Algorithms and Associated False Alarms. Swalwell B; Dalla S; Walsh RW Sol Phys; 2017; 292(11):173. PubMed ID: 31983778 [TBL] [Abstract][Full Text] [Related]
50. The FIELDS Instrument Suite for Solar Probe Plus: Measuring the Coronal Plasma and Magnetic Field, Plasma Waves and Turbulence, and Radio Signatures of Solar Transients. Bale SD; Goetz K; Harvey PR; Turin P; Bonnell JW; de Wit TD; Ergun RE; MacDowall RJ; Pulupa M; Andre M; Bolton M; Bougeret JL; Bowen TA; Burgess D; Cattell CA; Chandran BDG; Chaston CC; Chen CHK; Choi MK; Connerney JE; Cranmer S; Diaz-Aguado M; Donakowski W; Drake JF; Farrell WM; Fergeau P; Fermin J; Fischer J; Fox N; Glaser D; Goldstein M; Gordon D; Hanson E; Harris SE; Hayes LM; Hinze JJ; Hollweg JV; Horbury TS; Howard RA; Hoxie V; Jannet G; Karlsson M; Kasper JC; Kellogg PJ; Kien M; Klimchuk JA; Krasnoselskikh VV; Krucker S; Lynch JJ; Maksimovic M; Malaspina DM; Marker S; Martin P; Martinez-Oliveros J; McCauley J; McComas DJ; McDonald T; Meyer-Vernet N; Moncuquet M; Monson SJ; Mozer FS; Murphy SD; Odom J; Oliverson R; Olson J; Parker EN; Pankow D; Phan T; Quataert E; Quinn T; Ruplin SW; Salem C; Seitz D; Sheppard DA; Siy A; Stevens K; Summers D; Szabo A; Timofeeva M; Vaivads A; Velli M; Yehle A; Werthimer D; Wygant JR Space Sci Rev; 2016 Dec; 204(1-4):49-82. PubMed ID: 29755144 [TBL] [Abstract][Full Text] [Related]
51. EVIDENCE FOR THE MAGNETIC BREAKOUT MODEL IN AN EQUATORIAL CORONAL-HOLE JET. Kumar P; Karpen JT; Antiochos SK; Wyper PF; Devore CR; Deforest CE Astrophys J; 2018 Feb; 854(2):. PubMed ID: 33867543 [TBL] [Abstract][Full Text] [Related]
52. Fine Structure in Solar Flares. Warren HP Astrophys J; 2000 Jun; 536(2):L105-L108. PubMed ID: 10859129 [TBL] [Abstract][Full Text] [Related]
53. Shock heating in numerical simulations of kink-unstable coronal loops. Bareford MR; Hood AW Philos Trans A Math Phys Eng Sci; 2015 May; 373(2042):. PubMed ID: 25897092 [TBL] [Abstract][Full Text] [Related]
54. Relating magnetic reconnection to coronal heating. Longcope DW; Tarr LA Philos Trans A Math Phys Eng Sci; 2015 May; 373(2042):. PubMed ID: 25897089 [TBL] [Abstract][Full Text] [Related]
55. TRACE and Yohkoh Observations of High-Temperature Plasma in a Two-Ribbon Limb Flare. Warren HP; Bookbinder JA; Forbes TG; Golub L; Hudson HS; Reeves K; Warshall A Astrophys J; 1999 Dec; 527(2):L121-L124. PubMed ID: 10577954 [TBL] [Abstract][Full Text] [Related]
56. What can large-scale magnetohydrodynamic numerical experiments tell us about coronal heating? Peter H Philos Trans A Math Phys Eng Sci; 2015 May; 373(2042):. PubMed ID: 25897097 [TBL] [Abstract][Full Text] [Related]
57. Sources of solar energetic particles. Vlahos L; Anastasiadis A; Papaioannou A; Kouloumvakos A; Isliker H Philos Trans A Math Phys Eng Sci; 2019 Jul; 377(2148):20180095. PubMed ID: 31079581 [TBL] [Abstract][Full Text] [Related]
58. High-frequency torsional Alfvén waves as an energy source for coronal heating. Srivastava AK; Shetye J; Murawski K; Doyle JG; Stangalini M; Scullion E; Ray T; Wójcik DP; Dwivedi BN Sci Rep; 2017 Mar; 7():43147. PubMed ID: 28256538 [TBL] [Abstract][Full Text] [Related]
59. Relation between Flare-associated X-Ray Ejections and Coronal Mass Ejections. Nitta N; Akiyama S Astrophys J; 1999 Nov; 525(1):L57-L60. PubMed ID: 10511513 [TBL] [Abstract][Full Text] [Related]
60. Simulations of Switchback, Fragmentation and Sunspot Pair in Chang CJ; Kiang JF Sensors (Basel); 2021 Jan; 21(2):. PubMed ID: 33467536 [TBL] [Abstract][Full Text] [Related] [Previous] [Next] [New Search]