Effect of receiver shape and volume on the Alzheimer disease for molecular communication via diffusion

The work of I. Isik and M. E. Tagluk was supported by the Inonu University Project of Scientific Research Unit (BAP) under the project number FBA-2018-1013. The authors thank HP Turkey section for providing a powerful computer for computational tasks in this study. The work of H.B. Yilmaz is supported by the Scientific and Technical Research Council of Turkey (TUBITAK) under grant no. 118C274. The work of I. Demirkol was supported by the Spanish Government, MINECO, through project RYC-2013-13029Peer ReviewedPostprint (published version

CASIMIR: a submillimeter heterodyne spectrometer for SOFIA

The CAltech Submillimeter Interstellar Medium Investigations Receiver (CASIMIR) is a multichannel, heterodyne spectrometer being developed for the Stratospheric Observatory for Infrared Astronomy (SOFIA). It has a very high resolution, up to a million, over the submillimeter and far-infrared wavelength range of 150 to 600 micrometers , or 2.0 to 0.5 THz. CASIMIR is extremely well suited to the investigation of both the galactic and extragalactic warm, approximately 100 K, interstellar medium. A combination of advanced SIS and Hot Electron Bolometers receivers will be used to cover this frequency range with very high sensitivity. CASIMIR will use only solid state local oscillators, with quasioptical coupling to the mixers. We present a description of the instrument and its capabilities, including detailed discussions of the receivers, local oscillators and IF systems