Study of coronal jets during solar minimum based on STEREO/SECCHI observations

A. R. Paraschiv; D. A. Lacatus; T. Badescu; M. G. Lupu; S. Simon; S. G. Sandu; M. Mierla; M. V. Rusu

doi:10.1007/s11207-010-9584-6

Study of coronal jets during solar minimum based on STEREO/SECCHI observations

A. R. Paraschiv, D. A. Lacatus, T. Badescu, M. G. Lupu, S. Simon, S. G. Sandu, M. Mierla, M. V. Rusu

Solar Frontiers

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Abstract

During the 2007 - 2008 minimum of solar activity, the internally occulted coronagraphs SECCHI-COR1 onboard the STEREO space mission recorded numerous jet-like ejections over a great range of latitudes. We have found more than 10000 white-light jets in the above-mentioned period. Sometimes they can be identified on the disk with bright points observed in ultraviolet images by EUVI. In this study we present a catalog consisting of jets observed by the SECCHI-COR1 instrument and their association with lower coronal activity (bright points, UV jets). Furthermore, their association with bright points in the context of previously proposed models is discussed. From the complete catalog we have selected 106 jets observed in both STEREO-A and STEREO-B images for which it is possible to derive their kinematics and point of origin.

Original language	English
Pages (from-to)	365-375
Number of pages	11
Journal	Solar Physics
Volume	264
Issue number	2
DOIs	https://doi.org/10.1007/s11207-010-9584-6
State	Published - 2010

Keywords

Corona, structures
Coronal holes
Jets
Solar wind

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10.1007/s11207-010-9584-6

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title = "Study of coronal jets during solar minimum based on STEREO/SECCHI observations",

abstract = "During the 2007 - 2008 minimum of solar activity, the internally occulted coronagraphs SECCHI-COR1 onboard the STEREO space mission recorded numerous jet-like ejections over a great range of latitudes. We have found more than 10000 white-light jets in the above-mentioned period. Sometimes they can be identified on the disk with bright points observed in ultraviolet images by EUVI. In this study we present a catalog consisting of jets observed by the SECCHI-COR1 instrument and their association with lower coronal activity (bright points, UV jets). Furthermore, their association with bright points in the context of previously proposed models is discussed. From the complete catalog we have selected 106 jets observed in both STEREO-A and STEREO-B images for which it is possible to derive their kinematics and point of origin.",

keywords = "Corona, structures, Coronal holes, Jets, Solar wind",

author = "Paraschiv, \{A. R.\} and Lacatus, \{D. A.\} and T. Badescu and Lupu, \{M. G.\} and S. Simon and Sandu, \{S. G.\} and M. Mierla and Rusu, \{M. V.\}",

year = "2010",

doi = "10.1007/s11207-010-9584-6",

language = "English",

volume = "264",

pages = "365--375",

journal = "Solar Physics",

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TY - JOUR

T1 - Study of coronal jets during solar minimum based on STEREO/SECCHI observations

AU - Paraschiv, A. R.

AU - Lacatus, D. A.

AU - Badescu, T.

AU - Lupu, M. G.

AU - Simon, S.

AU - Sandu, S. G.

AU - Mierla, M.

AU - Rusu, M. V.

PY - 2010

Y1 - 2010

N2 - During the 2007 - 2008 minimum of solar activity, the internally occulted coronagraphs SECCHI-COR1 onboard the STEREO space mission recorded numerous jet-like ejections over a great range of latitudes. We have found more than 10000 white-light jets in the above-mentioned period. Sometimes they can be identified on the disk with bright points observed in ultraviolet images by EUVI. In this study we present a catalog consisting of jets observed by the SECCHI-COR1 instrument and their association with lower coronal activity (bright points, UV jets). Furthermore, their association with bright points in the context of previously proposed models is discussed. From the complete catalog we have selected 106 jets observed in both STEREO-A and STEREO-B images for which it is possible to derive their kinematics and point of origin.

AB - During the 2007 - 2008 minimum of solar activity, the internally occulted coronagraphs SECCHI-COR1 onboard the STEREO space mission recorded numerous jet-like ejections over a great range of latitudes. We have found more than 10000 white-light jets in the above-mentioned period. Sometimes they can be identified on the disk with bright points observed in ultraviolet images by EUVI. In this study we present a catalog consisting of jets observed by the SECCHI-COR1 instrument and their association with lower coronal activity (bright points, UV jets). Furthermore, their association with bright points in the context of previously proposed models is discussed. From the complete catalog we have selected 106 jets observed in both STEREO-A and STEREO-B images for which it is possible to derive their kinematics and point of origin.

KW - Corona, structures

KW - Coronal holes

KW - Jets

KW - Solar wind

UR - https://www.scopus.com/pages/publications/77954735202

U2 - 10.1007/s11207-010-9584-6

DO - 10.1007/s11207-010-9584-6

M3 - Article

AN - SCOPUS:77954735202

SN - 0038-0938

VL - 264

SP - 365

EP - 375

JO - Solar Physics

JF - Solar Physics

IS - 2

ER -

Study of coronal jets during solar minimum based on STEREO/SECCHI observations

Abstract

Keywords

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