Search Results - "Veronig, A"

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  1. 1

    Statistics of Coronal Dimmings Associated with Coronal Mass Ejections. II. Relationship between Coronal Dimmings and Their Associated CMEs by Dissauer, K., Veronig, A. M., Temmer, M., Podladchikova, T.

    Published in The Astrophysical journal (01-04-2019)
    “…We present a statistical study of 62 coronal dimming events associated with Earth-directed coronal mass ejections (CMEs) during the quasi-quadrature period of…”
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  2. 2

    Statistics of Coronal Dimmings Associated with Coronal Mass Ejections. I. Characteristic Dimming Properties and Flare Association by Dissauer, K., Veronig, A. M., Temmer, M., Podladchikova, T., Vanninathan, K.

    Published in The Astrophysical journal (20-08-2018)
    “…Coronal dimmings, localized regions of reduced emission in the extreme-ultraviolet and soft X-rays (SXRs), are interpreted as density depletions due to mass…”
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  3. 3

    Magnetic Reconnection Rates and Energy Release in a Confined X-class Flare by Veronig, A. M., Polanec, W.

    Published in Solar physics (01-10-2015)
    “…We study the energy-release process in the confined X1.6 flare that occurred on 22 October 2014 in AR 12192. Magnetic-reconnection rates and reconnection…”
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  4. 4

    On the Detection of Coronal Dimmings and the Extraction of Their Characteristic Properties by Dissauer, K., Veronig, A. M., Temmer, M., Podladchikova, T., Vanninathan, K.

    Published in The Astrophysical journal (10-03-2018)
    “…Coronal dimmings are distinct phenomena associated with coronal mass ejections (CMEs). The study of coronal dimmings and the extraction of their characteristic…”
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  5. 5

    Preconditioning of Interplanetary Space Due to Transient CME Disturbances by Temmer, M., Reiss, M. A., Nikolic, L., Hofmeister, S. J., Veronig, A. M.

    Published in The Astrophysical journal (01-02-2017)
    “…Interplanetary space is characteristically structured mainly by high-speed solar wind streams emanating from coronal holes and transient disturbances such as…”
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  6. 6

    Propagation of Interplanetary Coronal Mass Ejections: The Drag-Based Model by Vršnak, B., Žic, T., Vrbanec, D., Temmer, M., Rollett, T., Möstl, C., Veronig, A., Čalogović, J., Dumbović, M., Lulić, S., Moon, Y.-J., Shanmugaraju, A.

    Published in Solar physics (01-07-2013)
    “…We present the “Drag-Based Model” (DBM) of heliospheric propagation of interplanetary coronal mass ejections (ICMEs). The DBM is based on the hypothesis that…”
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  7. 7

    Combined STEREO/RHESSI Study of Coronal Mass Ejection Acceleration and Particle Acceleration in Solar Flares by Temmer, M, Veronig, A. M, Kontar, E. P, Krucker, S, Vršnak, B

    Published in The Astrophysical journal (01-04-2010)
    “…Using the potential of two unprecedented missions, Solar Terrestrial Relations Observatory (STEREO) and Reuven Ramaty High-Energy Solar Spectroscopic Imager…”
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  8. 8

    ASYMMETRY IN THE CME-CME INTERACTION PROCESS FOR THE EVENTS FROM 2011 FEBRUARY 14-15 by TEMMER, M, Veronig, A M, PEINHART, V, Vrsnak, B

    Published in The Astrophysical journal (20-04-2014)
    “…We present a detailed study of the interaction process of two coronal mass ejections (CMEs) successively launched on 2011 February 14 (CME1) and 2011 February…”
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  9. 9

    Understanding the Physical Nature of Coronal “EIT Waves” by Long, D. M., Bloomfield, D. S., Chen, P. F., Downs, C., Gallagher, P. T., Kwon, R.-Y., Vanninathan, K., Veronig, A. M., Vourlidas, A., Vršnak, B., Warmuth, A., Žic, T.

    Published in Solar physics (01-01-2017)
    “…For almost 20 years the physical nature of globally propagating waves in the solar corona (commonly called “EIT waves”) has been controversial and subject to…”
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  10. 10

    STEREO Quadrature Observations of the Three-Dimensional Structure and Driver of a Global Coronal Wave by Kienreich, I. W, Temmer, M, Veronig, A. M

    Published in The Astrophysical journal (01-10-2009)
    “…We present the first observations of a global coronal wave ('EIT wave') from the two STEREO satellites in quadrature. The wave's initiation site was at the…”
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  11. 11

    An Observational Overview of Solar Flares by Fletcher, L., Dennis, B. R., Hudson, H. S., Krucker, S., Phillips, K., Veronig, A., Battaglia, M., Bone, L., Caspi, A., Chen, Q., Gallagher, P., Grigis, P. T., Ji, H., Liu, W., Milligan, R. O., Temmer, M.

    Published in Space science reviews (01-09-2011)
    “…We present an overview of solar flares and associated phenomena, drawing upon a wide range of observational data primarily from the RHESSI era. Following an…”
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  12. 12

    Microflares and the Statistics of X-ray Flares by Hannah, I. G., Hudson, H. S., Battaglia, M., Christe, S., Kašparová, J., Krucker, S., Kundu, M. R., Veronig, A.

    Published in Space science reviews (01-09-2011)
    “…This review surveys the statistics of solar X-ray flares, emphasising the new views that RHESSI has given us of the weaker events (the microflares). The new…”
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  13. 13

    IMPULSIVE ACCELERATION OF CORONAL MASS EJECTIONS. II. RELATION TO SOFT X-RAY FLARES AND FILAMENT ERUPTIONS by BEIN, B. M, BERKEBILE-STOISER, S, VERONIG, A. M, TEMMER, M, VRSNAK, B

    Published in The Astrophysical journal (10-08-2012)
    “…Using high time cadence images from the STEREO EUVI, COR1, and COR2 instruments, we derived detailed kinematics of the main acceleration stage for a sample of…”
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  14. 14

    Impulsive Acceleration of Coronal Mass Ejections. I. Statistics and Coronal Mass Ejection Source Region Characteristics by Bein, B. M, Berkebile-Stoiser, S, Veronig, A. M, Temmer, M, Muhr, N, Kienreich, I, Utz, D, Vršnak, B

    Published in The Astrophysical journal (10-09-2011)
    “…We use high time cadence images acquired by the STEREO EUVI and COR instruments to study the evolution of coronal mass ejections (CMEs) from their initiation…”
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  15. 15

    Initiation of Coronal Mass Ejections by Sunspot Rotation by Török, T., Temmer, M., Valori, G., Veronig, A. M., van Driel-Gesztelyi, L., Vršnak, B.

    Published in Solar physics (01-09-2013)
    “…We study a filament eruption, two-ribbon flare, and coronal mass ejection (CME) that occurred in NOAA Active Region 10898 on 6 July 2006. The filament was…”
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  16. 16

    STEREO and Wind observations of a fast ICME flank triggering a prolonged geomagnetic storm on 5-7 April 2010 by Möstl, C., Temmer, M., Rollett, T., Farrugia, C. J., Liu, Y., Veronig, A. M., Leitner, M., Galvin, A. B., Biernat, H. K.

    Published in Geophysical research letters (01-12-2010)
    “…On 5 April 2010 an interplanetary (IP) shock was detected by the Wind spacecraft ahead of Earth, followed by a fast (average speed 650 km/s) IP coronal mass…”
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  17. 17

    Acceleration in Fast Halo CMEs and Synchronized Flare HXR Bursts by Temmer, M, Veronig, A. M, Vršnak, B, Rybák, J, Gömöry, P, Stoiser, S, Maričić, D

    Published in The Astrophysical journal (20-01-2008)
    “…We study two well-observed, fast halo CMEs, covering the full CME kinematics including the initiation and impulsive acceleration phase, and their associated…”
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  18. 18

    Statistical Properties of Ribbon Evolution and Reconnection Electric Fields in Eruptive and Confined Flares by Hinterreiter, J., Veronig, A. M., Thalmann, J. K., Tschernitz, J., Pötzi, W.

    Published in Solar physics (01-03-2018)
    “…A statistical study of the chromospheric ribbon evolution in H α two-ribbon flares was performed. The data set consists of 50 confined (62%) and eruptive (38%)…”
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  19. 19

    CONNECTING SPEEDS, DIRECTIONS AND ARRIVAL TIMES OF 22 CORONAL MASS EJECTIONS FROM THE SUN TO 1 AU by MOSTL, C, AMLA, K, Hall, J R, LIEWER, P C, de Jong, E M, COLANINNO, R C, Veronig, A M, Rollett, T, TEMMER, M, PEINHART, V

    Published in The Astrophysical journal (01-06-2014)
    “…Forecasting the in situ properties of coronal mass ejections (CMEs) from remote images is expected to strongly enhance predictions of space weather and is of…”
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  20. 20

    Relation Between Coronal Hole Areas on the Sun and the Solar Wind Parameters at 1 AU by Rotter, T., Veronig, A. M., Temmer, M., Vršnak, B.

    Published in Solar physics (01-12-2012)
    “…We analyze the relationship between the coronal hole (CH) characteristics on the Sun (area, position, and intensity levels) and the corresponding solar wind…”
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