What are the plasma parameters (n,T,v, |B|) in the ambient (pre-shocked) corona? ... White light coronagraphy (SOHO/LASCO, MLSO) UV coronal spectroscopy (SOHO ...
The proposed aim of this study seeks to extract quantitative parameters from ... analysis moved forward, we became increasingly aware of glaring inconsistencies ...
Contrary to this, sunspot activity may be correlated with the climate on Earth. In the period between 1645 and 1715, sunspot activity had come to a halt on the Sun – a phenomenon referred to as the Maunder minimum.
It is important to understand the difference between coronal polishing and a ... Patients who are at high risk for dental caries. Sensitive Teeth. Newly erupted teeth ...
(Webb et al., 1994; Gosling, 1990; Williams et al., 2005) Typical energy: ... (MacQueen et al., 1974, Hildner et al., 1975, Gosling et al., 1976) Tempel, 1860 ...
... the Sun (part of the corona is expelled with its magnetic field) ... corona ... modern sense (OSO-7): Tousey, R., The solar corona, Adv. Space Res., 13,713, 1973. ...
Nevertheless several clear observations of coronal sources 20 keV have been reported ... Review by Cliver et al., ApJ 305, 920 (1986) Coronal sources of hard X-rays? ...
Some nice picture. Some nice pictures (continued) 20 July 2002. X3.3 flare on ... Hard X-ray source extends to 20-30'' over limb which when added to occultation ...
collapsing magnetic trap is the same for Fermi and betatron. mechanism. However, trap with dominant betatron acceleration confines particles better ...
CME interaction: Cannibalism or deflection depending on the separation between solar sources ... (Cannibalism) 830 km/s. 1460 km/s. 1999 09 03: Radio Emission ...
... search has been driven by wave-based coronal heating theories. Few consistent observations in hot material ... EIT and TRACE imaging - 1998, 1999, 2000 - new ...
Skylab coronagraph/Ulysses in-situ. Heliocentric distance / Rs ... Low density, n 108 cm-3, consistent with coronagraph measurements. hot protons, Tmax 5 M K ...
Global coronal seismology and EIT waves. Istvan Ballai. SP2RC, University of Sheffield, UK ... Coronal seismology. Local seismology: using waves propagating in ...
Coronal loop oscillations and diagnostics with Hinode/EIS. Youra Taroyan ... methods currently used in coronal seismology rely on the presence of coherent ...
Last brightening is footprint of CME leg. Model:expanding flux rope. Delann e et al. (in press) ... They are possibly signature of opening of magnetic field ...
Measurement of coronal magnetic fields - Radio diagnosis as one possibility ... Millisecond radio spikes on Nov 2, 1997 (Huang, 2004) Nobeyama Symposium, 2004 ...
Figure 6.1: Adult with an enhancing intrasellar tumor with suprasellar extension. ... as eosinophilic adenoma giving rise to gigantism/acromegaly and ACTH producing ...
NASA Goddard Space Flight Center, Greenbelt, Maryland ... apex with solar North. Width = PA2 PA1. Speed = dh/dt. W. S. N. PA1. PA2. CPA (h,t) Height-Time Plot ...
los. r2. Summary. Taking advantage of the unique characteristics of STEREO to: Calculate real' v ... los. r2. Acceleration of the Jet. Other Examples of ...
... region, left upper panel 'transition region', bottom panel 'coronal region' ... (x = L/2) bottom left (right) panel; all for mass density contrast d = 108, ...
The problem of accounting for the combined influence exerted ... It is quite clear, however, that in some cases regular refraction ... photosphere. source ...
Initiative on the use of Coronal Magnetic Field measurements in theoretical ... Look for polarization signatures of quasi-separatrix surfaces in the solar corona ...
With results from A. Van Ballegooijen, A. Winebarger and H. Warren ... 1. Why is the corona hot? 2. Why is the corona structured? ... coronal seismology ...
ON THE RELATION BETWEEN FILAMENT ERUPTIONS, FLARES, AND CORONAL MASS EJECTIONS ... CMEs --- LASCO C2 coronagraph images and the CME catalog to determine. ...
The solar corona is a high temperature and low plasma where the magnetic field ... Intensit (image de gauche) de la raie 1074.7 nm du Fe XIII et quantit ...
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 ...
Yohkoh X-Ray image. Coronal hole. Active. region. Quiet. region ... Yohkoh X-Ray image. Coronal hole. heavy ions (e.g., O 5) are hotter than protons and electrons: ...
vector field from a bipolar Active region (number 1731) on. February 21, 2002 ... This line profile is one of the first measurements of a 30G coronal magnetic field ...
Task 1B: measure and map the magnetic free energy ... IX: Business plan: Resources ... X: Business plan: Implementation [Define key milestones, test procedures, ...
Eric Priest suggests that if we can determine the temperature profiles along the ... EIT (Extreme Ultraviolet Imaging Telescope) CDS (Coronal Diagnostic Spectrometer) ...
Originally discovered via soft X-ray images (see also Waldmeier's ' ... appear when a new active region emerges within a CH boundary (rosette or anemone) ...
Development is an integral part of the Sun's magnetic-field evolution ... mass is brought up from the chromosphere: jets, levitation, or evaporation ...
SoHO MDI. SoHO MDI. White light. Line-of-sight B. 2001 Aug 11, 11:15 UT. Aug 16, 2004 ... SoHO MDI. movie. Aug 16, 2004. Magnetic evolution. Aug 16, 2004. Aug ...
The National Center for Atmospheric Research is operated by ... Soft-x ray observation from Yohkoh. Pevtsov, Canfield, & Latushko (2001) Canfield et al. (1999) ...
... for Coronal Magnetic Field Measurements by EUV and X-ray Spectroscopy. Sophie Canton (Charge exchange) Matt Carpenter (Algorithms,CX) Jaan Lepson (EUV spectra) ...