Coronal separatrix structure. The separatrix surfaces deform ... that the separatrix structure. correlated in interesting ways. with the in-plane motions, ...
Time evolution is represented by the brightness. The first interval is the. darkest one. ... Comparision between several models of density (Aschwanden et al. 2002) and ...
They are also often asymmetric in size and magnetic field ... The size of the footpoint should be ... Old algorithms don't weight size sensitivity properly ...
In plage, Diffuse but some 'kernels' More SXR emission at footpoints. ... At footpoints in plage. Magnetic field strength (Gauss) Magnetic field inclination ...
The Yohkoh observations of solar flares Hugh Hudson UCB The Yohkoh observations Structure in soft X-rays Dynamics in soft X-rays Footpoint behavior Coronal hard X-ray ...
A null and the associated separatrix. Continuous footpoint motion of. At the photosphere boundary ... on the separatrix. Force-free equilibrium. The growth rate ...
Jets, Outflows and Disks all seem part of high mass star formation (Shepherd, ... provide views of 'meso-scale' jets. Jet rotation - disk footpoints (Ray et ...
Corona B at photosphere. Global relation between AR corona and magnetic fields has been well studied. Magnetic Flux ... Non-uniformity in AR corona ...
Measuring the Temperature of Hot Solar Flare Plasma with RHESSI Amir Caspi1,2, Sam Krucker2, Robert P. Lin1,2 1 Department of Physics, University of California ...
?? 2 may be explained by an intermediate situation between the two extremes. ... seems to be at work, differing in one flare for the two legs of the loop. ...
Feb. 2006. HMI/AIA Science Team Mtg. 1. Heating the Corona and Driving the Solar Wind ... Feb. 2006. HMI/AIA Science Team Mtg. 2. Coronal Heating. The corona ...
Yohkoh Hard X-ray Telescope gave for the first time an opportunity for massive ... for HXRs (e.g. Frost & Dennis 1971, stereo-scopic papers of Kane) ...
3. DSM/DAPNIA/Service d'Astrophysique, CEA Saclay, France ... Collaborators: A. A. Van Ballegooijen, E. E. Deluca, J. McCaughey, K. K. Reeves, and M. Gros ...
Lee et al 2000, - dynamics of spectral properties, electron anisotropy ... Fleishman & Melnikov 2003, - influence of electron pitch angle anisotropy ...
From detailed magneto-convection simulations to modelling the ... Institute of Theoretical Astrophysics, University of Oslo. Monterey February 14 2006 ...
Construct X-ray and EUV false images. Compare with observations ... Empirical relationship from Pevtsov et al. soft x-ray data. Solve Static Energy Equation: ...
RHESSI Observations of Super-Hot (T 30 MK) Plasma in Large Solar Flares Amir Caspi1 & Robert P. Lin1 1 Department of Physics & Space Sciences Laboratory,
Electron Acceleration at the Solar Flare Reconnection Outflow Shocks. Gottfried Mann, Henry Aurass, and ... dynamic radio spectrogram height-time diagram ...
Richard Nightingale. James Lemen (LMSAL) 2nd SECCHI/STEREO Meeting, Abingdon, UK, 2001 July 12-13. The Goal ... Create a set of synthetic EUVI image pairs that ...
S. Masuda (STEL, Nagoya Univ.) TOF analysis (Aschwanden et al. 1996) ... Low-frequency component: trap and precipitation. Ne = 1 - 2 1011 cm-3. Trapping region ...
collapsing magnetic trap is the same for Fermi and betatron. mechanism. However, trap with dominant betatron acceleration confines particles better ...
Magnetic helicity is a conserved quantity even. in resistive MHD (Berger, 1984) ... magnetograph & spectrograph. fov: 164'x164', Blong=1-5 G, Btrans=30-50 G. temp. ...
Dept. of Astronomy, University of Maryland, College Park, MD and Lab for ... Time profiles of 17GHz and X-Ray time profile and spectrogram. 2002 May 03 ...
ultaneously at INTERBALL-2 and on the Ground. 3 November 1996, 23: ... inkangas, S. Perrault, et al. Paperin alareunasta 2 cm pois. SOD. IT-2. 23:00 UT. 23:30 UT ...
Accretion Channeling in CTTS. Scott Gregory, Moira Jardine. Classical T ... (e.g. Guenther et al. 1999). Electron-cyclotron maser emission (Smith et al. 2003) ...
stop near the separatrix between active regions and thus appear as a stationary front ... The EIT wave stopped near the separatrix. Discussion. Model of the EIT wave ...
In this poster, we compare various methods for interpolation of ... flux transportation model based method (data from Schrijver and DeRosa, 2002). Method 1 ...
... div B = 0. Demand that there be no singularities and that ... That is, find p(r), Jp(r), and Jt(r). Describe the physical meaning of the parameter q? ...
Ratio of EIT full Sun images in Fe XII 195A to Fe IX/X 171A ... sheets: tangential discontinuity which become increasingly severe with the ... A Hybrid Shell Model ...
TENACIOUS: Tomographic ENA Comprehensive Ion+Optical University Satellite Robert Sheldon, UAH, T.Fritz, H.Spence, J.Sullivan, J.Vickers, D.Cotton, M.Alothman, BU
Coronal loop oscillations and diagnostics with Hinode/EIS. Youra Taroyan ... methods currently used in coronal seismology rely on the presence of coherent ...
Solar Flares are often classified into two types: compact flares and two ribbon flares. ... (2) Supra-Arcade Downflows in LDEs. ITP Workshop Jan-18-2002 ...
Observational evidence of coronal oscillations (or quasi-periodic pulsations) is ... Possible relevance to coronal heating and solar wind acceleration problems. ...
Thermal and nonthermal contributions to the solar flare X-ray flux ... Thin Shutters In (A1) Detector #4. 1-minute accumulations. RHESSI Count-rate Spectrum ...
MAGNETIC TWIST OF EUV CORONAL LOOPS. OBSERVED BY TRACE. RyunYoung Kwon, ... There is a tendency that the twist in the middle of the loop is larger than both ...
Pickup Ions and Reservoir for Energetic Particles George Gloeckler & Eberhard M bius PUI Session PUI Production Rates Didkowski et al. PUI Sources Drews et al ...
Plasma velocities observed with CDS during impulsive phase of 2 flares ... CDS observations with slit above a rising filament magnetic field extrapolations ...