Fig. 1
From: Observation based climatology Martian atmospheric waves perturbation Datasets
Dataset creation process. Based on the input data (third column) collected by instruments (second column) of spacecrafts (first column), the output data (final column) is reconstructed using DINEOF method. The spacecrafts used include the orbiters (MRO, MGS, MEX, and MAVEN) and the landers (MP, MPL, MER1, and MER2). They are connected to the detection instruments (MCS, TES, RO, SPICAM, IUVS, ASI/MET, and IMU) they carry by polylines. The arrows connected to each instrument point to the data type (limb viewing data, nadir viewing data, radio occultation data, solar occultation data, stellar occultation data, and entry accelerometers data) they provide. The output data (MAWPD) is the reconstructed climatology gridded temperature data (Level 1 data) and the derived gravity waves, tides, and stationary planetary waves (Level 2 data).
