REPORT FROM ISAS 6-May-94 to 17-May-94 D. Alexander This week was a week of mixed fortune. After all our hard work in preparing for the May 10 Eclipse we were thwarted by some big time bad luck. Basically, we were hit by an SEU (Single Event Upset) which is another TLA (Three Letter Acronym) for a CRE (Cosmic Ray Event). This caused an SXT error which meant we were unable to upload the appropriate SXT tables. None of our planned experiments succeeded, although we did get a couple of eclipse images at around 14:10 UT as well as some coronal images round the time of the San Diego eclipse observations. The BCS,unfortunately, did not fair any better since the count rate was very low. In addition an OP error resulted in the overwriting of some of the BCS data. All in all it was a valuable, if disappointing, experience and if the Sun complies we will try again in November. This week sees the start of the Chromospheric Ejection Campaign with Brigitte Schmieder of Meudon and collaborators. There is currently an interesting active region on the solar disk and this should provide some good observations over the next week. This campaign will run until June 3. Giovanni Peres gave a very interesting talk on the 12th. He is using the hydro-code of the Palermo loop to compare various heating mechanisms in flaring loops with the details of the SXT observations. In particular, he has been able to reproduce some of the observed spatial variations for some simple events. This approach is potentially quite important since it allows us to check what physics are appropriate in different types of flaring loop and to provide possible diagnostic tests for the heating of these loops. Marilyn Bruner has been working hard on the analysis of her rocket data, both the recent flight and the '92 flight. In preparation for the upcoming AGU meeting, Marilyn has produced a coaligned data set which includes SXT, CIV, Ly-alpha together with UV continuum and La Palma data (H-alpha, H-alpha wing, visible continuum and magnetogram). The results of this will be reported in Baltimore. The recent rocket flight has yielded cleaner spectra than the '92 flight and sveral good images of the Sun at a number of wavelengths. In particular, there are good UV spectra as well as some EUV lines, good 171A images (essentially FeIX) which provides data at temperatures intermediate between SXT and CIV data. There are excellent Ly-alpha images showing many prominences at the limb and these are being compared with SXT Full Frame Images. Hugh Hudson, Greg Slater and I have been looking at the Polar Crown event which occurred on April 14 this year. This event is the one which produced a large enhancement of the geomagnetic activity at the Earth some days later. We are preparing a number of images of this event for use at the IACG meeting, to be held here at ISAS at the end of the month, where we hope to discuss the general nature of large scale solar structures. We are particularly interested in the long term behaviour of such structures and whether we can determine if the large scale magnetic field configuration existed prior to the heating witnessed by SXT or if the heating was a side effect of the reconfiguration of the magnetic field. Sarah Matthews and Norman Gray arrive tomorrow from the University of Glasgow. Under their influence I will probably slip into my native mode of speaking and will start to speak even more quickly than I do at present. Yecannywhackit! JOKE OF THE MONTH How many solar physicists does it take to change a fuse? 44, 1 to change the fuse, 1 to switch on the light and 42 to argue about whether the loop reconnected or not. QUOTE OF THE WEEK "If there is a word in the dictionary under any letter from A to Z that I abominate, it is energy. It is such a conventional superstition, such parrot gabble" Dickens, "Our Mutual Friend" ERRATA: In the last report there was a glaring grammatical error. Please correct 'by Hugh Hudson and I' to 'by I and Hugh Hudson'. In this report please replace 'errata' with 'erratum'.