Basics & Motivation Technique & Observations Fits & Measurements Summary & Outlook Atmospheric Wave Workshop ESTEC 11/10/2011 Tobias Stangier I st Physics.
Non renewable Renewable Pancha Bhoothas SKYWATERLANDFIREAIR.
Geostationary Lightning Mapper (GLM) 1 Near uniform spatial resolution of approximately 10 km. Coverage up to 52 deg latitude. 70-90% flash detection day.
Introduction to the sky. On a clear, moonless night, far from city lights, the night sky is magnificent. Roughly 2000 stars are visible to the unaided.
Solar Site Assessment Why the variation in solar radiation? Amount of atmosphere sun’s energy must travel through to reach earth – Time of day, Time.
Solar Sources of Earth-affecting Energetic Particles
Lecture 3 read Hartmann Ch.2 and A&K Ch.2 Brief review of blackbody radiation Earth’s energy balance TOA: top-of-atmosphere –Total flux in (solar or SW)=
AERO2K Global Aviation Emissions Inventories for 2002 and 2025.
JEM/SMILES Mission
WIND RESOURCE ASSESSMENT TECHNIQUES
DoDAF 2.0 Exemplars UPDM 1.0 X DoDAF 2.0 X DM2 PES XML Examples 12 August 2010 DoDAF Development Team.
