The only difference is that the maximum values of N e measured by Swarm are now spread on a wider longitude sector including also the Atlantic Ocean.
This likely indicates the strong Northern Hemisphere sources that contribute over wide longitude ranges to the loadings but is also due, in part, to relatively poor profile statistics in HIPPO 1, which provides the lowest average rBC MMR here; the single highest altitude HIPPO1 rBC MMR value in this latitude band is based on two profiles, while the next highest was based on four.
In middle and low latitudes the spectral peak at 1.6 mHz was a common feature in wide longitudes, but the 3.5 mHz peak was not detected in the forenoon region.
Because little is known about the population genetics of E. roseum, which covers a wide range of longitudes and climates, we cannot exclude the possibility that these samples represent cryptic species.
We have also coadded groups of five images to increase signal to noise and plotted in Figure 2a the intensity averaged over the 30°-wide longitude sector indicated by the yellow meridians in Figures 1a– 1f, versus colatitude.
The common peak is found at 1.6 mHz in ground spectra in a wide region of geomagnetic longitude from 310° to 33° (GDH through CBB) in the forenoon to noon sector.
However, the Pi1, Pi1-2 and Pi2 arrival patterns are quite dissimilar across a wide range of latitudes and longitudes.
According to a few in situ satellite observations, the disturbed region extends across a wide range of latitudes and longitudes (Oyama et al. 2008), such as 60° in the East West (EW) direction and 40° in the North South (NS) direction for large EQs of M > 6.
He sees jazz as a wide grid: a 100-year-old longitude and a latitude that extends to Michael Jackson, Sun Ra and free improvising.
Multi-site measurements of interplanetary scintillation (IPS) can provide information on solar wind velocity at any heliolatitude or longitude and over a wide range of heliocentric distances, with the coverage limited only by the availability of suitable radio sources and the geometry of the observing system.
