We use calibrated extreme-UV (EUV) spectral irradiances obtained from observations with the Solar & Heliospheric Observatory (SOHO) Coronal Diagnostics Spectrometer Normal Incidence Spectrometer (NIS) to estimate the signal measured by the Solar EUV Monitor (SEM) first-order band, 260 to 340 Å (SEM 1). The NIS observes the resonance lines He i
The solar EUV irradiance is a key input for thermospheric and ionospheric models. Difficulties in c...
abstract EGU05-A-08437The solar EUV flux is a key quantity for studying solar-terrestrial interactio...
After discussing the methods of observation, solar EUV flux measurements are reviewed. In spite of t...
We use calibrated extreme-UV (EUV) spectral irradiances obtained from observations with the Solar & ...
We present extreme-ultraviolet (EUV) irradiances of the Sun taken during the 1998–2010 period from t...
We present SOHO Coronal Diagnostic Spectrometer (CDS) normal incidence, extreme-ultraviolet spectra...
We present calibrated EUV spectral irradiances obtained from observations with the Solar and Heliosp...
We benchmark new atomic data against a selection of irradiances obtained from medium-resolution quie...
An in-flight calibration study of the Coronal Diagnostic Spectrometer (CDS) instrument on board SOH...
The solar Extreme UltraViolet (EUV) spectrum has important effects on the Earth’s upper atmosphere. ...
For the first time, we present and discuss EUV radiances of the solar transition region (TR) and cor...
For the first time, we present and discuss EUV radiances of the solar transition region (T...
The Extreme Ultraviolet (EUV) irradiance central and first order channel time series (COC and FOC) f...
Meeting abstract from the CDROM, #991The severe lack of continuously measured and spectrally resolve...
International audienceWe use recent solar extreme ultraviolet (EUV) irradiance data from the Solar E...
The solar EUV irradiance is a key input for thermospheric and ionospheric models. Difficulties in c...
abstract EGU05-A-08437The solar EUV flux is a key quantity for studying solar-terrestrial interactio...
After discussing the methods of observation, solar EUV flux measurements are reviewed. In spite of t...
We use calibrated extreme-UV (EUV) spectral irradiances obtained from observations with the Solar & ...
We present extreme-ultraviolet (EUV) irradiances of the Sun taken during the 1998–2010 period from t...
We present SOHO Coronal Diagnostic Spectrometer (CDS) normal incidence, extreme-ultraviolet spectra...
We present calibrated EUV spectral irradiances obtained from observations with the Solar and Heliosp...
We benchmark new atomic data against a selection of irradiances obtained from medium-resolution quie...
An in-flight calibration study of the Coronal Diagnostic Spectrometer (CDS) instrument on board SOH...
The solar Extreme UltraViolet (EUV) spectrum has important effects on the Earth’s upper atmosphere. ...
For the first time, we present and discuss EUV radiances of the solar transition region (TR) and cor...
For the first time, we present and discuss EUV radiances of the solar transition region (T...
The Extreme Ultraviolet (EUV) irradiance central and first order channel time series (COC and FOC) f...
Meeting abstract from the CDROM, #991The severe lack of continuously measured and spectrally resolve...
International audienceWe use recent solar extreme ultraviolet (EUV) irradiance data from the Solar E...
The solar EUV irradiance is a key input for thermospheric and ionospheric models. Difficulties in c...
abstract EGU05-A-08437The solar EUV flux is a key quantity for studying solar-terrestrial interactio...
After discussing the methods of observation, solar EUV flux measurements are reviewed. In spite of t...
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