Proposal ID Pres_176

Date of Proposal May 29 1998

firstname

Pawel

lastname

Pres

institute

Rutherford Appleton Laboratory

address

Space Science Division
Rutherford Appleton Laboratory
Chilton, Didcot, Oxon. 0X11 0QX
U.K.

email

pres@solg2.bnsc.rl.ac.uk

phone

+44 1235 446497

fax

+44 1235 446667

proposal

We are comparing the X-ray and EUV emission together with
magnetic field measurements from the quiet Sun network structure
for the time period between the 31 July and 1 August 1997. We have
found some spatial and temporal correlation between magnetic
changes and X-ray and EUV emission which we believe to be very
significant in terms of previous findings about X-ray network
flares or blinkers.

For SoHO, we are using data sets from MDI, EIT and CDS
instruments. For the case of CDS we are analysing the data from
the FLARE and NTBRMDI1 study. For SXT, we are using the full
frame images as well as the partial frames (10'x10').

inside_collab

consortium

yes

topic

Bright Points

topic

title

SXT and SoHO quiet Sun images comparison

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