lofar - Swedish Institute of Space Physics - Uppsala

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Field vectors across an antenna array for a radio beam with orbital angular momentum Phase 0 deg Phase 45 deg B. Thidé et al., preprint, 2005 Bo Thidé 44 EISCAT Radar School, Kiruna,, 2005
EM beams with orbital angular momentum (OAM) l=+1 l=+3 l= -4 Courtesy and © M. J. Padgett, J. Leach et al., U. Glasgow, UK; Royal Society Bo Thidé 45 EISCAT Radar School, Kiruna,, 2005
Page 1 and 2: Physics in Space Programme LOFAR Ou
Page 3 and 4: Hydrogen radiates at 1420.4 MHz (21
Page 5 and 6: Q1: How to observe 21 cm line radio
Page 7 and 8: Predicted EoR spectrum to test Big
Page 9 and 10: Bo Thidé 9 EISCAT Radar School, Ki
Page 11 and 12: Sensor field Fibre data transport C
Page 13 and 14: First LOFAR ITS results Bo Thidé 1
Page 15 and 16: LOFAR Phase 2 into Lower Saxony, Sc
Page 17 and 18: Three orthogonal linear dipole ante
Page 19 and 20: LOIS resources Supercomputer cluste
Page 21 and 22: LOIS and LOFAR Bo Thidé 21 EISCAT
Page 23 and 24: LOFAR and LOIS concept • Combine
Page 25 and 26: Secondary radiation experiment setu
Page 27 and 28: LOIS/LOFAR beat-wave excitation mod
Page 29 and 30: HF pump frequency dependence Pump f
Page 31 and 32: Secondary ionospheric radiation/SEE
Page 33 and 34: SEE diagnostic of Langmuir turbulen
Page 35 and 36: Polarimetric signatures of the HF p
Page 37 and 38: 3D polarimetry utilising that E(t,x
Page 39 and 40: EM symmetries (continued) Bo Thidé
Page 41 and 42: EM beam with spin (circular polaris
Page 43: Helical radio beams carry orbital a
Page 47 and 48: OAM as a new RF modulation techniqu
Page 49 and 50: Bo Thidé 49 EISCAT Radar School, K
Page 51 and 52: Ultra-High Energy Particle Detectio
Page 53: Radio methods If wavelength is long

lofar - Swedish Institute of Space Physics - Uppsala

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