Inference of the Local Interstellar Spectra of Cosmic-Ray Nuclei Z ≤ 28 with the GALPROP-HELMOD Framework

Composition and spectra of Galactic cosmic rays (CRs) are vital for studies of high-energy processes in a variety of environments and on different scales, for interpretation of gamma-ray and microwave observations, for disentangling possible signatures of new phenomena, and for understanding of our local Galactic neighborhood. Since its launch, AMS-02 has delivered outstanding-quality measurements of the spectra of (p) over bar, e(+/-), and nuclei: H-1-O-8, Ne-10, Mg-12, Si-14. These measurements resulted in a number of breakthroughs; however, spectra of heavier nuclei and especially low-abundance nuclei are not expected until later in the mission. Meanwhile, a comparison of published AMS-02 results with earlier data from HEAO-3-C2 indicates that HEAO-3-C2 data may be affected by undocumented systematic errors. Utilizing such data to compensate for the lack of AMS-02 measurements could result in significant errors. In this paper we show thata fractionof HEAO-3-C2 datamatchavailable AMS-02 measurements quite well and can be used together with Voyager 1 and ACE-CRIS data to makepredictionsfor the local interstellar spectra (LIS) of nuclei that are not yet released by AMS-02. We are also updating our already-published LIS to provide a complete set from(1) H-(28) Ni in the energy range from 1 MeV nucleon(-1) to similar to 100-500 TeV nucleon(-1), thus covering 8-9 orders of magnitude in energy. Our calculations employ the GalProp-HelModframework, which has proved to be a reliable tool in deriving the LIS of CR (p) over bar, e(-), and nuclei H-1-O-8.