The Solar-B Mission and the Forefront of Solar Physics

By T. Sakurai, T. Sekii. 2004

202 citations recorded by the source corpus.

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

Differential Emission Measures from the Regularized Inversion of Hinode and SDO data (2012, unknown): “(Weber et al. 2004; Golub et al. 2004).”
DIFFERENTIAL EMISSION MEASURE ANALYSIS OF MULTIPLE STRUCTURAL COMPONENTS OF CORONAL MASS EJECTIONS IN THE INNER CORONA (2012, methodology): “This code was originally designed for Hinode/XRT (X-ray Telescope) data (Golub et al. 2004; Weber et al. 2004), and here is modified slightly to work with AIA data (see also Schmelz et al. 2010, 2011a,b; Winebarger et al. 2011).”
Tracking Vector Magnetograms with the Magnetic Induction Equation (2008, methodology): “In the interest of reproducibility (Joyner & Stein 2007), all of the software used to perform the calculations, create the figures, and draw the conclusions for this paper can be found in the electronic edition of the Journal as a tgz file.”
Simulating and Predicting Solar Cycles Using a Flux-Transport Dynamo (2006, background): “(d,e,f) Additional flux emerges (d,e) and spreads (f) in latitude and longitude from decaying spots (as described in figure 5 of Babcock (1961)). (g) Meridional flow (yellow circulation with arrows) carries surface magnetic flux poleward, causing polar fields to reverse. (h) Some of this flux is the”
The Solar Optical Telescope for the Hinode Mission: An Overview (2007, background): “Convective collapse (Parker, 1978) may form the kilogauss-strength tubes and eventually form pores and sunspots from weaker emerging fields.”