Search Publications

Explosive Events: Swirling Transition Region Jets
DOI: 10.1007/s11207-012-9940-9 Bibcode: 2012SoPh..280..417C

Curdt, W.; Tian, H.; Kamio, S.

In this paper, we extend our earlier work to provide additional evidence for an alternative scenario to explain the nature of events called `explosive events'. The bidirected, fast Doppler motion of explosive events observed spectroscopically in the transition region emission is classically interpreted as a pair of bidirectional jets moving upward…

2012 Solar Physics
Hinode SOHO 36
Three-Dimensional Properties of Coronal Mass Ejections from STEREO/SECCHI Observations
DOI: 10.1007/s11207-012-0123-5 Bibcode: 2012SoPh..281..167B

Davies, J. A.; Bothmer, V.; Howard, R. A. +3 more

We identify 565 coronal mass ejections (CMEs) between January 2007 and December 2010 in observations from the twin STEREO/SECCHI/COR2 coronagraphs aboard the STEREO mission. Our list is in full agreement with the corresponding SOHO/LASCO CME Catalog (http://cdaw.gsfc.nasa.gov/CME_list/) for events with angular widths of 45 and up. The …

2012 Solar Physics
SOHO 35
Oscillations in Active Region Fan Loops: Observations from EIS/ Hinode and AIA/SDO
DOI: 10.1007/s11207-012-0098-2 Bibcode: 2012SoPh..281...67K

Banerjee, D.; Krishna Prasad, S.; Singh, Jagdev

Active region fan loops in AR 11076 were studied, in search of oscillations, using high cadence spectroscopic observations from Extreme-ultraviolet Imaging Spectrometer (EIS) on board Hinode combined with imaging sequences from the Atmospheric Imaging Assembly (AIA) on board Solar Dynamics Observatory (SDO). Spectra from EIS were analyzed in two s…

2012 Solar Physics
Hinode 35
Coronal Mass Ejections from Magnetic Systems Encompassing Filament Channels Without Filaments
DOI: 10.1007/s11207-011-9881-8 Bibcode: 2012SoPh..277..185P

Pevtsov, Alexei A.; Panasenco, Olga; Martin, Sara F.

Well-developed filament channels may be present in the solar atmosphere even when there is no trace of filament material inside them. Such magnetic systems with filament channels without filaments can result in coronal mass ejections that might appear to have no corresponding solar surface source regions. In this case study, we analyze CMEs on 9 A…

2012 Solar Physics
SOHO 29
Uncovering the Birth of a Coronal Mass Ejection from Two-Viewpoint SECCHI Observations
DOI: 10.1007/s11207-012-9933-8 Bibcode: 2012SoPh..280..509V

Tsinganos, K.; Vourlidas, A.; Syntelis, P.

We investigate the initiation and formation of Coronal Mass Ejections (CMEs) via a detailed two-viewpoint analysis of low corona observations of a relatively fast CME acquired by the SECCHI instruments aboard the STEREO mission. The event which occurred on 2 January 2008, was chosen because of several unique characteristics. It shows upward motion…

2012 Solar Physics
SOHO 25
The Creation of Outflowing Plasma in the Corona at Emerging Flux Regions: Comparing Observations and Simulations
DOI: 10.1007/s11207-011-9855-x Bibcode: 2012SoPh..278...47H

van Driel-Gesztelyi, L.; Harra, L. K.; Hood, A. W. +3 more

In this paper we analyse the flux emergence that occurred in the following polarity area of an active region on 1 - 2 December 2006. Observations have revealed the existence of fast outflows at the edge of the emerging flux region. We have performed 3-D numerical simulations to study the mechanisms responsible for these flows. The results indicate…

2012 Solar Physics
Hinode SOHO 25
The Free Energy of NOAA Solar Active Region AR 11029
DOI: 10.1007/s11207-011-9878-3 Bibcode: 2012SoPh..276..133G

Leka, K. D.; Wheatland, M. S.; Gilchrist, S. A.

The NOAA active region (AR) 11029 was a small but highly active sunspot region which produced 73 GOES soft X-ray flares during its transit of the disk in late October 2009. The flares appear to show a departure from the well-known power law frequency-size distribution. Specifically, too few GOES C-class and no M-class flares were observed by compa…

2012 Solar Physics
Hinode 24
On Signatures of Twisted Magnetic Flux Tube Emergence
DOI: 10.1007/s11207-011-9789-3 Bibcode: 2012SoPh..278...33V

van Driel-Gesztelyi, L.; Vargas Domínguez, S.; MacTaggart, D. +2 more

Recent studies of NOAA active region 10953, by Okamoto et al. (Astrophys. J. Lett.673, 215, 2008; Astrophys. J.697, 913, 2009), have interpreted photospheric observations of changing widths of the polarities and reversal of the horizontal magnetic field component as signatures of the emergence of a twisted flux tube within the active region and al…

2012 Solar Physics
SOHO 22
Scientific Analysis within SEPServer - New Perspectives in Solar Energetic Particle Research: The Case Study of the 13 July 2005 Event
DOI: 10.1007/s11207-012-0164-9 Bibcode: 2012SoPh..281..333M

Vainio, R.; Valtonen, E.; Riihonen, E. +19 more

Solar energetic particle (SEP) events are a key ingredient of solar-terrestrial physics both for fundamental research and space weather applications. Multi-satellite observations are an important and incompletely exploited tool for studying the acceleration and the coronal and interplanetary propagation of the particles. While STEREO uses for this…

2012 Solar Physics
SOHO 22
Modeling and Interpreting the Effects of Spatial Resolution on Solar Magnetic Field Maps
DOI: 10.1007/s11207-011-9821-7 Bibcode: 2012SoPh..277...89L

Leka, K. D.; Barnes, G.

Different methods for simulating the effects of spatial resolution on magnetic field maps are compared, including those commonly used for inter-instrument comparisons. The investigation first uses synthetic data, and the results are confirmed with Hinode/SpectroPolarimeter data. Four methods are examined, one which manipulates the Stokes spectra t…

2012 Solar Physics
Hinode SOHO 22