The Incoherent Scatter Radar (ISR) at the European Incoherent SCATter (EISCAT) has been in operation since 1981. The transmitter and one receiver is at Tromso, Norway (69.58N, 19.23E) at the approximate apex magentic latitude of 66.4 magN, and so is often in the auroral zone. At 300 km the IGRF B magnitude is 0.4687 gauss, with inclination angle of 77.997 deg and declination angle of 4.538. There are two other receivers for bistatic operation at Kiruna, sweden (67.87N, 20.43E) and in Sodankyla, Finland (67.37N, 26.63W). These are all UHF receivers, where a separate VHF receiver and transmitter is located at Tromso. The EISCAT Svalbard Radar (ESR) on Svalbard Island, Norway has been in operation since 1996 at (75.15N, 16.05E) at the approximate apex magentic latitude of 75.0 magN, and so is often in the polar cap. At 300 km the IGRF B magnitude is 0.4822 gauss, with inclination angle of 82.236 deg and declination angle of 2.5870. Plots and data for both ISRs are available at http://www.eiscat.se/madrigal in the EISCAT node of the Madrigal Database. The contact person is Esa Turunen (esa.turunen@eiscat.se). Another possible EISCAT contact who is in charge of World-Day scheduling is Ingemar Haggstrom (ingemar@eiscat.se, 46-(980)-79155, Fax 46-(980)-79159, EISCAT Scientific Association, Box 812, SE-98128 Kiruna, Sweden). Please contact them early to confirm correct use of the ISR data and to offer co-authorship for any publications. ACKNOWLEDGMENTS: We are indebted to the Director and staff of EISCAT for operating the facility and supplying the data. EISCAT is an international association supported by Finland (SA, Suomen Akatemia), France (CNRS, Centre National de la Recherche Scientifique), Germany (MPG, Max-Planck-Gesellschaft), Japan (NIPR, National Institute for Polar Research), Norway (NFR, Norges forskningsrad), Sweden (NFR, Naturvetensckapliga forskningsradet), and the United Kingdom (PPARC, Particle Physics and Astronomy Research Council). These data for the joint GEM-CEDAR Challenge of 2011 were taken from kindat=6800, which used 3 separate positions as tau1 (20 deg elevation at the Tromso UHF site), tau2 (77.5 deg elevation at the Tromso UHF site, where the other 2 UHF sites were used to get electric field vectors), and tau8 (30 deg elevation at the Tromso VHF site). The tau2 77.5 deg elevation data had 42 altitudes from 76-674 km. Only 32 altitudes from 106-674 km were retained. At Svalbard, the 42m data were labelled tau0 at 81.6 deg elevation for 53 altitudes between 78-1253 km. Only 31 altitudes from 102-613 km were retained. Both ISR data sets were around 1 minute with a fine height resolution power profile (for uncorrected Ne with kindat 6801) at the same time. We used the tau2 Tromso data and tau0 Svalbard data with corrected Ne (in m-3), Te (as Te/Ti), Ti (in K), and line-of-sight (LOS) ion velocity, which is similar to Wi for elev 77 and 82. The Ne data were retained if the Ne error bar was less than the Ne value. The Ti, Te, and LOS drift data were retained if the temperature error bars were <200 K, if Te/Ti were between 0.2 and 5.0, and if Ti>500K for ht>300km. The LOS drift data with error bars >200 m/s were also deleted. The GEM-CEDAR Challenge included the values of LOS Vi (~Wi), Ne, Te, and Ti near 250 km (at 246+/-~20km) from kindat 6800 in files labelled eis(or esr)_...20m_profiles. Approximately 20 EISCAT and 10 Svalbard 1-min profiles were averaged every 20 min to improve the data quality, where the error bars were the standard deviations. If only 1 value was in the average at a particular height, the error bar was the original error bar. The maximum Ne value (Nmax in m-3) was found in each averaged profile between 100-600 km at height hmax (km). If a polynomial fit could be made, Nmax and hmax were refined. The total electron content (TEC in m-2) was found between 100-600 km. Nmax and Nmax were not always in the F-region, and TEC will be added later, so none of the variables in the eis(or esr)_..._20m_nmax files were used in the GEM-CEDAR Challenge. The analyst for making these 20-min data was Barbara Emery of HAO/NCAR.