145 related articles for article (PubMed ID: 37483848)
1. Transverse oscillations and an energy source in a strongly magnetized sunspot.
Yuan D; Fu L; Cao W; Kuźma B; Geeraerts M; Trelles Arjona JC; Murawski K; Van Doorsselaere T; Srivastava AK; Miao Y; Feng S; Feng X; Noda CQ; Cobo BR; Su J
Nat Astron; 2023; 7(7):856-866. PubMed ID: 37483848
[TBL] [Abstract][Full Text] [Related]
2. Transverse motions in sunspot super-penumbral fibrils.
Morton RJ; Mooroogen K; Henriques VMJ
Philos Trans A Math Phys Eng Sci; 2021 Feb; 379(2190):20200183. PubMed ID: 33342382
[TBL] [Abstract][Full Text] [Related]
3. 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]
4. Evidence for wave heating in the solar corona.
Hahn M
Ann N Y Acad Sci; 2013 Jul; 1293():45-53. PubMed ID: 23676178
[TBL] [Abstract][Full Text] [Related]
5. Observations of ubiquitous compressive waves in the Sun's chromosphere.
Morton RJ; Verth G; Jess DB; Kuridze D; Ruderman MS; Mathioudakis M; Erdélyi R
Nat Commun; 2012; 3():1315. PubMed ID: 23271649
[TBL] [Abstract][Full Text] [Related]
6. Evidence of ubiquitous Alfvén pulses transporting energy from the photosphere to the upper chromosphere.
Liu J; Nelson CJ; Snow B; Wang Y; Erdélyi R
Nat Commun; 2019 Aug; 10(1):3504. PubMed ID: 31383869
[TBL] [Abstract][Full Text] [Related]
7. Magnetoacoustic cutoff effect in numerical simulations of the partially ionized solar atmosphere.
Kuźma B; Kadowaki LHS; Murawski K; Musielak ZE; Poedts S; Yuan D; Feng X
Philos Trans A Math Phys Eng Sci; 2024 Jun; 382(2272):20230218. PubMed ID: 38679054
[TBL] [Abstract][Full Text] [Related]
8. 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]
9. Recent advances in coronal heating.
De Moortel I; Browning P
Philos Trans A Math Phys Eng Sci; 2015 May; 373(2042):. PubMed ID: 25897095
[TBL] [Abstract][Full Text] [Related]
10. High-frequency acoustic waves are not sufficient to heat the solar chromosphere.
Fossum A; Carlsson M
Nature; 2005 Jun; 435(7044):919-21. PubMed ID: 15959510
[TBL] [Abstract][Full Text] [Related]
11. 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]
12. Solar chromospheric spicules from the leakage of photospheric oscillations and flows.
De Pontieu B; Erdélyi R; James SP
Nature; 2004 Jul; 430(6999):536-9. PubMed ID: 15282598
[TBL] [Abstract][Full Text] [Related]
13. Spectropolarimetric fluctuations in a sunspot chromosphere.
Stangalini M; Baker D; Valori G; Jess DB; Jafarzadeh S; Murabito M; To ASH; Brooks DH; Ermolli I; Giorgi F; MacBride CD
Philos Trans A Math Phys Eng Sci; 2021 Feb; 379(2190):20200216. PubMed ID: 33342387
[TBL] [Abstract][Full Text] [Related]
14. A substantial amount of hidden magnetic energy in the quiet Sun.
Bueno JT; Shchukina N; Ramos AA
Nature; 2004 Jul; 430(6997):326-9. PubMed ID: 15254531
[TBL] [Abstract][Full Text] [Related]
15. Three-dimensional magnetic field topology in a region of solar coronal heating.
Solanki SK; Lagg A; Woch J; Krupp N; Collados M
Nature; 2003 Oct; 425(6959):692-5. PubMed ID: 14562096
[TBL] [Abstract][Full Text] [Related]
16. Generation of solar spicules and subsequent atmospheric heating.
Samanta T; Tian H; Yurchyshyn V; Peter H; Cao W; Sterling A; Erdélyi R; Ahn K; Feng S; Utz D; Banerjee D; Chen Y
Science; 2019 Nov; 366(6467):890-894. PubMed ID: 31727839
[TBL] [Abstract][Full Text] [Related]
17. Alfven waves in the solar corona.
Tomczyk S; McIntosh SW; Keil SL; Judge PG; Schad T; Seeley DH; Edmondson J
Science; 2007 Aug; 317(5842):1192-6. PubMed ID: 17761876
[TBL] [Abstract][Full Text] [Related]
18. Magnetoacoustic wave energy dissipation in the atmosphere of solar pores.
Gilchrist-Millar CA; Jess DB; Grant SDT; Keys PH; Beck C; Jafarzadeh S; Riedl JM; Van Doorsselaere T; Ruiz Cobo B
Philos Trans A Math Phys Eng Sci; 2021 Feb; 379(2190):20200172. PubMed ID: 33342383
[TBL] [Abstract][Full Text] [Related]
19. Flare differentially rotates sunspot on Sun's surface.
Liu C; Xu Y; Cao W; Deng N; Lee J; Hudson HS; Gary DE; Wang J; Jing J; Wang H
Nat Commun; 2016 Oct; 7():13104. PubMed ID: 27721463
[TBL] [Abstract][Full Text] [Related]
20. Resolved magnetohydrodynamic wave lensing in the solar corona.
Zhou X; Shen Y; Yuan D; Keppens R; Zhao X; Fu L; Tang Z; Wang J; Zhou C
Nat Commun; 2024 Apr; 15(1):3281. PubMed ID: 38627403
[TBL] [Abstract][Full Text] [Related]
[Next] [New Search]
