Observational Evidences for Extremely Strong Magnetic Fields in Solar Flares

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International Journal of Astronomy and Astrophysics

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"Observational Evidences for Extremely Strong Magnetic Fields in Solar Flares"
written by Vsevolod Gryhorovych Lozitsky,
published by International Journal of Astronomy and Astrophysics, Vol.1 No.3, 2011

has been cited by the following article(s):

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[1]	Signatures of superstrong magnetic fields in a limb solar flare from observations of the Hα line
	Advances in Space Research, 2022

[2]	ESTIMATIONS OF LOCAL MAGNETIC FIELDS IN SOLAR FLARES: BASIC METHODS AND SOME RESULTS
	2017

[3]	MAGNETIC FIELDS AND THERMODYNAMICAL CONDITIONS AT PHOTOSPHERIC LAYERS OF X17. 2/4B SOLAR FLARE OF 28 OCTOBER 2003
	2017

[4]	МАГНІТНІ ПОЛЯ В ПРОТОННОМУ СОНЯЧНОМУ СПАЛАХУ БАЛУ Х17. 2/4B ЗА ДАНИМИ ОДНОЧАСНИХ ВИМІРЮВАНЬ У КІЛЬКОХ СПЕКТРАЛЬНИХ …
	2017

[5]	MAGNETIC FIELDS IN POWERFUL SOLAR FLARES AT LEVELS OF PHOTOSPHERE AND CHROMOSPHERE
	2017

[6]	ПОРІВНЯННЯ ХРОМОСФЕРНИХ І ФОТОСФЕРНИХ МАГНІТНИХ ПОЛІВ У ДВОХ СОНЯЧНИХ СПАЛАХАХ БАЛІВ Х1. 1/4N І X17. 2/4B
	2017

[7]	Magnetic fields in proton solar flare of X17.2/4B class according to data of simultaneous measurements in a few spectral lines
	Bulletin of Taras Shevchenko National University of Kyiv. Astronomy, 2017

[8]	Comparison of chromospheric and photospheric magnetic fields in two solar flares of X1. 1/4N and X17. 2/4B importance
	2017

[9]	Вимірювання магнітних полів у сонячних плямах по спектральних лініях з різними факторами Ланде
	2017

[10]	Earth atmosphere grazing meteors
	2017

[11]	Магнітні поля в протонному сонячному спалаху БАЛУ Х17. 2/4B за даними одночасних вимірювань в кількох спектральних лініях
	2017

[12]	Порівняння хромосферних і фотосферних магнітних полів у двох сонячних спалахах балів х1. 1/4n та x17. 2/4b
	2017

[13]	A Mathematical Model of the Maximum Rigidity Resulting from Diffusive Shock Acceleration
	2016

[14]	Small-scale magnetic field diagnostics in solar flares using bisectors of I±V profiles
	Advances in Space Research, 2015

[15]	Indications of 8-kilogauss magnetic field existence in the sunspot umbra
	Advances in Space Research, 2015

[16]	SIMULTANEOUS MAGNETIC FIELD MEASUREMENTS IN SUNSPOTS USING SPECTRAL LINES WITH DIFFERENT LANDE FACTORS
	Odessa Astronomical Publications, 2015

[17]	Якою є максимальна напруженість локальних магнітних полів в активних протуберанцях?
	Вісн. Київ. нац. ун-ту імені Тараса Шевченка. Астрономія, 2014

[18]	Small-scale magnetic field diagnostics in solar flares using bisectors of I± V profiles
	Advances in Space Research, 2014

[19]	Chromospheric Magnetic Field Measurements in a Flare and an Active Region Filament
	Solar Physics, 2012

[20]	COMPARATIVE STUDY OF SPECTRAL LINES WITH DIFFERENT LANDE FACTORS OBSERVED IN SUNSPOTS


[21]	INDICATIONS OF SUPERSTRONG MAGNETIC FIELDS IN A LIMB SOLARE FLARE AND AN ACTIVE PROMINENCE FROM SPECTRO-POLARIMETRIC

[1]	Signatures of superstrong magnetic fields in a limb solar flare from observations of the Hα line Advances in Space Research, 2022 DOI:10.1016/j.asr.2022.04.012

[2]	Comparative study of spectral lines with different Landé factors observed in sunspots Journal of Physical Studies, 2022 DOI:10.30970/jps.26.4902

[3]	Indications of 8-kilogauss magnetic field existence in the sunspot umbra Advances in Space Research, 2016 DOI:10.1016/j.asr.2015.08.032

[4]	Small-scale magnetic field diagnostics in solar flares using bisectors of I±V profiles Advances in Space Research, 2015 DOI:10.1016/j.asr.2014.09.028

[5]	Chromospheric Magnetic Field Measurements in a Flare and an Active Region Filament Solar Physics, 2012 DOI:10.1007/s11207-012-0067-9

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