58 research outputs found
Nova light curves from the Solar Mass Ejection Imager (SMEI) - II. The extended catalog
We present the results from observing nine Galactic novae in eruption with the Solar Mass Ejection Imager (SMEI) between 2004 and 2009. While many of these novae reached peak magnitudes that were either at or approaching the detection limits of SMEI, we were still able to produce light curves that in many cases contained more data at and around the initial rise, peak, and decline than those found in other variable star catalogs. For each nova, we obtained a peak time, maximum magnitude, and for several an estimate of the decline time (t2). Interestingly, although of lower quality than those found in Hounsell et al. (2010a), two of the light curves may indicate the presence of a pre-maximum halt. In addition the high cadence of the SMEI instrument has allowed the detection of low amplitude variations in at least one of the nova light curves
CME 3D Reconstructions Using Solar Mass Ejection Imager and Interplanetary Scintillation Data
Solar Mass Ejection Imager (SMEI) 3-D Reconstructions of CMEs, CIRs and Interplanetary Shocks, and Comparison with In-situ Data
Solar Wind Speed Inferred from Cometary Plasma Tails using Observations from STEREO HI-1
About the Solar Mass Ejection Imager (SMEI) 3D-Reconstruction-and-Display of Co-rotating Heliospheric Structure during the Present Deep Solar Minimum
Inclusion of In-Situ Velocity Measurements into the UCSD Time-Dependent Tomography to Constrain and Better-Forecast Remote-Sensing Observations
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