Scan of specimen UMMZ:mammals:112964 (Desmodus rotundus) - WholeBody. Raw Dataset includes 3141 TIF images (each 1047 x 1326 x 1 voxel at 0.04145749 mm resolution, derived from 3141 scan projections), xtek and vgi files for volume reconstruction. and Scan of specimen UMMZ:mammals:112964 (Desmodus rotundus) - WholeBody. Reconstructed Dataset includes 2000 TIF images (each 1047 x 1326 x 1 voxel at 0.041457 mm resolution, derived from 3141 scan projections), xtek and vgi files for volume reconstruction.
Scan of specimen UMMZ:herps:130609 (PHAEOGNATHUS HUBRICHTI) - WholeBody. Raw Dataset includes 1601 TIF images (each 373 x 372 x 1 voxel at 0.1000025 mm resolution, derived from 1601 scan projections), xtek and vgi files for volume reconstruction. and Scan of specimen UMMZ:herps:130609 (PHAEOGNATHUS HUBRICHTI) - WholeBody. Reconstructed Dataset includes 2000 TIF images (each 373 x 372 x 1 voxel at 0.100002 mm resolution, derived from 1601 scan projections), xtek and vgi files for volume reconstruction.
Scan of specimen ummz:mammals:154691 (Blarina brevicauda brevicauda) - Skull. Reconstructed Dataset includes 1035 TIF images (each 1322 x 910 x 1 voxel at 0.027133 mm resolution, derived from 3141 scan projections), xtek and vgi files for volume reconstruction. and Scan of specimen ummz:mammals:154691 (Blarina brevicauda brevicauda) - Skull. Raw Dataset includes 3141 TIF images (each 1322 x 910 x 1 voxel at 0.02713322 mm resolution, derived from 3141 scan projections), xtek and vgi files for volume reconstruction.
Scan of specimen ummz:mammals:154691 (Blarina brevicauda brevicauda) - WholeBody. Raw Dataset includes 3141 TIF images (each 1187 x 834 x 1 voxel at 0.03976336 mm resolution, derived from 3141 scan projections), xtek and vgi files for volume reconstruction. and Scan of specimen ummz:mammals:154691 (Blarina brevicauda brevicauda) - WholeBody. Reconstructed Dataset includes 2000 TIF images (each 1187 x 834 x 1 voxel at 0.039763 mm resolution, derived from 3141 scan projections), xtek and vgi files for volume reconstruction.
Scan of specimen ummz:mammals:166889 (Blarina brevicauda kirtlandi) - Skull. Raw Dataset includes 3141 TIF images (each 1570 x 1531 x 1 voxel at 0.01919876 mm resolution, derived from 3141 scan projections), xtek and vgi files for volume reconstruction. and Scan of specimen ummz:mammals:166889 (Blarina brevicauda kirtlandi) - Skull. Reconstructed Dataset includes 1978 TIF images (each 1570 x 1531 x 1 voxel at 0.019199 mm resolution, derived from 3141 scan projections), xtek and vgi files for volume reconstruction.
Scan of specimen ummz:mammals:166889 (Blarina brevicauda kirtlandi) - WholeBody. Raw Dataset includes 3141 TIF images (each 877 x 1047 x 1 voxel at 0.03681702 mm resolution, derived from 3141 scan projections), xtek and vgi files for volume reconstruction. and Scan of specimen ummz:mammals:166889 (Blarina brevicauda kirtlandi) - WholeBody. Reconstructed Dataset includes 1882 TIF images (each 877 x 1047 x 1 voxel at 0.036817 mm resolution, derived from 3141 scan projections), xtek and vgi files for volume reconstruction.
Scan of specimen ummz:mammals:154693 (Blarina brevicauda brevicauda) - Skull. Reconstructed Dataset includes 1219 TIF images (each 1013 x 1693 x 1 voxel at 0.033795 mm resolution, derived from 3141 scan projections), xtek and vgi files for volume reconstruction. and Scan of specimen ummz:mammals:154693 (Blarina brevicauda brevicauda) - Skull. Raw Dataset includes 3141 TIF images (each 1013 x 1693 x 1 voxel at 0.03379497 mm resolution, derived from 3141 scan projections), xtek and vgi files for volume reconstruction.
This data set was created with the purpose to study the electron pitch angle distributions on dayside closed crustal fields at Mars and to compare with theoretical predictions made by numerical modeling. Analyzing the plasma environment of the crustal fields was another point of study to determine if whistler waves can interact with high energy superthermal electrons.
Amiri-Farahani, A., Olson, N. E., Neubauer, D., Roozitalab, B., Ault, A. P., & Steiner, A. L. (2021). Lake Spray Aerosol Emissions Alter Nitrogen Partitioning in the Great Lakes Region. Geophysical Research Letters, 48(12), e2021GL093727. https://doi.org/10.1029/2021GL093727
A new empirical model of the plasmapause location has been developed using density data from the plasma wave receiver onboard the CRRES spacecraft for nearly 1000 orbits. The “plasmapause” is identified here as the innermost sharp gradient in density (change of a factor of 5 in <0.5 L). Such a sharp gradient was observed on 73% of the CRRES inbound and outbound orbits that returned data. The plasmapause location is expressed as a linear function of Kp (previous 12 hour maximum) and local time. The model gives the linear best fit location of the plasmapause as well as the standard deviations of the model parameters.
Moldwin, M. B., Downward, L., Rassoul, H. K., Amin, R., and Anderson, R. R. (2002), A new model of the location of the plasmapause: CRRES results, J. Geophys. Res., 107( A11), 1339, doi:10.1029/2001JA009211 and O'Brien, T. P., and Moldwin, M. B. (2003), Empirical plasmapause models from magnetic indices, Geophys. Res. Lett., 30, 4, 1152. doi:10.1029/2002GL016007