Erratum: "Inference of the Local Interstellar Spectra of Cosmic-Ray Nuclei Z ⩽ 28 with the GALPROP-HELMOD Framework" (2020, ApJS, 250, 27).

[This corrects the article PMC8549769.].

The Discovery of a Low-energy Excess in Cosmic-Ray Iron: Evidence of the Past Supernova Activity in the Local Bubble.

Since its launch, the Alpha Magnetic Spectrometer-02 (AMS-02) has delivered outstanding quality measurements of the spectra of cosmic-ray (CR) species ( p ¯ , e ±, and nuclei, 1H-8O, 10Ne, 12Mg, 14Si) which resulted in a number of breakthroughs. One of the latest long-awaited surprises is the spectrum of 26Fe just published by AMS-02. Because of the large fragmentation cross section and large ionization energy losses, most of CR iron at low energies is local and may harbor some features associated with relatively recent supernova (SN) activity in the solar neighborhood. Our analysis of the new AMS-02 results, together with Voyager 1 and ACE-CRIS data, reveals an unexpected bump in the iron spectrum and in the Fe/He, Fe/O, and Fe/Si ratios at 1-2 GV, while a similar feature in the spectra of He, O, and Si and in their ratios is absent, hinting at a local source of low-energy CRs. The found excess extends the recent discoveries of radioactive 60Fe deposits in terrestrial and lunar samples and in CRs. We provide an updated local interstellar spectrum (LIS) of iron in the energy range from 1 MeV nucleon-1 to ~10 TeV nucleon-1. Our calculations employ the GALPROP-HELMOD framework, which has proved to be a reliable tool in deriving the LIS of CR p ¯ , e -, and nuclei Z ⩽ 28.

Deciphering the Local Interstellar Spectra of Secondary Nuclei with the Galprop/Helmod Framework and a Hint for Primary Lithium in Cosmic Rays.

Local interstellar spectra (LIS) of secondary cosmic-ray (CR) nuclei, lithium, beryllium, boron, and partially secondary nitrogen, are derived in the rigidity range from 10 MV to ~200 TV using the most recent experimental results combined with state-of-the-art models for CR propagation in the Galaxy and in the heliosphere. The lithium spectrum appears somewhat flatter at high energies compared to other secondary species, which may imply a primary lithium component. Two propagation packages, GALPROP and HelMod, are combined to provide a single framework that is run to reproduce direct measurements of CR species at different modulation levels, and at both polarities of the solar magnetic field. An iterative maximum-likelihood method is developed that uses GALPROP-predicted LIS as input to HelMod, which provides the modulated spectra for specific time periods of the selected experiments for the model-data comparison. The proposed LIS accommodates the low-energy interstellar spectra measured by Voyager 1, the High Energy Astrophysics Observatory-3 (HEAO-3), and the Cosmic Ray Isotope Spectrometer on board of the Advanced Composition Explorer (ACE/CRIS), as well as the high-energy observations by the Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics (PAMELA), Alpha Magnetic Spectrometer-02 (AMS-02), and earlier experiments that are made deep in the heliosphere. The interstellar and heliospheric propagation parameters derived in this study are consistent with our earlier results for propagation of CR protons, helium, carbon, oxygen, antiprotons, and electrons.

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 γ-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 ¯ , e ±, and nuclei: 1H-8O, 10Ne, 12Mg, 14Si. 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 that a fraction of HEAO-3-C2 data match available AMS-02 measurements quite well and can be used together with Voyager 1 and ACE-CRIS data to make predictions for 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 1H-28Ni in the energy range from 1 MeV nucleon-1 to ~100-500 TeV nucleon-1, thus covering 8-9 orders of magnitude in energy. Our calculations employ the GalProp-HelMod framework, which has proved to be a reliable tool in deriving the LIS of CR p ¯ , e -, and nuclei 1H-8O.

HelMod in the Works: From Direct Observations to the Local Interstellar Spectrum of Cosmic-Ray Electrons.

The local interstellar spectrum (LIS) of cosmic-ray (CR) electrons for the energy range 1 MeV to 1 TeV is derived using the most recent experimental results combined with the state-of-the-art models for CR propagation in the Galaxy and in the heliosphere. Two propagation packages, GALPROP and HelMod, are combined to provide a single framework that is run to reproduce direct measurements of CR species at different modulation levels, and at both polarities of the solar magnetic field. An iterative maximum-likelihood method is developed that uses GALPROP-predicted LIS as input to HelMod, which provides the modulated spectra for specific time periods of the selected experiments for model-data comparison. The optimized HelMod parameters are then used to adjust GALPROP parameters to predict a refined LIS with the procedure repeated subject to a convergence criterion. The parameter optimization uses an extensive data set of proton spectra from 1997 to 2015. The proposed CR electron LIS accommodates both the low-energy interstellar spectra measured by Voyager 1 as well as the high-energy observations by PAMELA and AMS-02 that are made deep in the heliosphere; it also accounts for Ulysses counting rate features measured out of the ecliptic plane. The interstellar and heliospheric propagation parameters derived in this study agree well with our earlier results for CR protons, helium nuclei, and anti-protons propagation and LIS obtained in the same framework.

Deciphering the Local Interstellar Spectra of Primary Cosmic-Ray Species with helmod.

Local interstellar spectra (LIS) of primary cosmic ray (CR) nuclei, such as helium, oxygen, and mostly primary carbon are derived for the rigidity range from 10 MV to ~200 TV using the most recent experimental results combined with the state-of-the-art models for CR propagation in the Galaxy and in the heliosphere. Two propagation packages, GALPROP and helmod, are combined into a single framework that is used to reproduce direct measurements of CR species at different modulation levels, and at both polarities of the solar magnetic field. The developed iterative maximum-likelihood method uses GALPROP-predicted LIS as input to helmod, which provides the modulated spectra for specific time periods of the selected experiments for model-data comparison. The interstellar and heliospheric propagation parameters derived in this study are consistent with our prior analyses using the same methodology for propagation of CR protons, helium, antiprotons, and electrons. The resulting LIS accommodate a variety of measurements made in the local interstellar space (Voyager 1) and deep inside the heliosphere at low (ACE/CRIS, HEAO-3) and high energies (PAMELA, AMS-02).

Solution of Heliospheric Propagation: Unveiling the Local Interstellar Spectra of Cosmic-ray Species.

Local interstellar spectra (LIS) for protons, helium, and antiprotons are built using the most recent experimental results combined with state-of-the-art models for propagation in the Galaxy and heliosphere. Two propagation packages, GALPROP and HelMod, are combined to provide a single framework that is run to reproduce direct measurements of cosmic-ray (CR) species at different modulation levels and at both polarities of the solar magnetic field. To do so in a self-consistent way, an iterative procedure was developed, where the GALPROP LIS output is fed into HelMod, providing modulated spectra for specific time periods of selected experiments to compare with the data; the HelMod parameter optimization is performed at this stage and looped back to adjust the LIS using the new GALPROP run. The parameters were tuned with the maximum likelihood procedure using an extensive data set of proton spectra from 1997 to 2015. The proposed LIS accommodate both the low-energy interstellar CR spectra measured by Voyager 1 and the high-energy observations by BESS, Pamela, AMS-01, and AMS-02 made from the balloons and near-Earth payloads; it also accounts for Ulysses counting rate features measured out of the ecliptic plane. The found solution is in a good agreement with proton, helium, and antiproton data by AMS-02, BESS, and PAMELA in the whole energy range.

Long-term study of TNBS-induced colitis in rats: focus on mast cells.

OBJECTIVE AND DESIGN: To investigate the severity and duration of colitis induced by two different doses of 2,4,6-trinitrobenzenesulfonic acid (TNBS) and the changes in mast cell number in acute inflammation and in the recovery process of colitis. METHODS: Colitis was induced in rats by an enema of TNBS (10 or 30 mg) in 25% ethanol. Macroscopic and histologic changes of the colon, colon weight and mast cell counts were examined at various times (7, 30 and 60 days) after colitis induction. RESULTS: TNBS induced a colonic damage which was dose-related for both severity and time necessary to complete recovery. On day 7 after colitis induction 10 mg TNBS induced macroscopic and microscopic alterations of colonic architecture that completely resolved at day 60. By contrast, 30 mg TNBS induced massive necrosis, thickening of the colon, severe histologic changes that were only partially reversed after two months. Mast cell number in the submucosa and muscularis propria decreased significantly in the acute phase of inflammation (7 days) and slowly increased thereafter, reaching a maximum level (up to about 5-fold) at day 60 after both doses of TNBS. CONCLUSIONS: Present data confirm the ability of TNBS to induce in rats damage to the colon that was dose-dependent for severity and duration. Moreover, these data unravel a different role of mast cells in TNBS-induced colitis: an early degranulation in the acute phase of inflammation and a subsequent accumulation of mast cells in the late phase of the disease, associated with tissue repair.

Morphological and functional alterations of the myenteric plexus in rats with TNBS-induced colitis.

The 2,4,6-trinitrobenzenesulfonic acid (TNBS)-induced model of experimental colitis was used to investigate the time-course of alterations in enteric neurotransmission and/or smooth muscle function that occur in chronic inflammation. Myenteric plexus morphology (immunocytochemical markers), functional integrity of cholinergic neurons (3H-choline uptake, acetylcholine release and contractile response to electrical field stimulation) and smooth muscle integrity (contractile response to exogenous acetylcholine) were determined 2, 7, 15, and 30 days after TNBS treatment. In TNBS-treated rats extensive ulcerations of the mucosa and/or the submucosa and increase in colonic weights were accompanied by significant reduction in 3H-choline uptake, acetylcholine release and contractile response to stimulation of enteric nerves. These changes were maximal 7 and 15 days after TNBS treatment. Immunocytochemical marker (PGP 9.5, SNAP 25, synaptophysin and S100 protein) expression was absent in necrotic areas of colons removed 7 days post-injury and partially reduced in colons removed 15 days after TNBS treatment. By contrast, the contractile response to exogenous acetylcholine was significantly increased after 7 days in both inflamed and uninflamed regions and returned to control values by day 30. Likewise, an almost complete recovery of neural cholinergic function and of myenteric plexus morphology was observed 30 days after TNBS treatment. These data suggest that TNBS-induced colitis is associated with progressive and selective alterations in myenteric plexus structure and function, with consequent reduction of cholinergic neurotransmission and abnormality in colonic contractility. The reversibility of myenteric plexus disruption is a clear indication of neuronal plasticity within enteric nervous system as an adaptative mechanism against inflammatory challenges.

Role of histamine H3 receptors in the regulation of gastric functions.

The role of central and peripheral histamine H3 receptors in the regulation of gastric acid secretion and gastric mucosal integrity is reviewed. The activation of H3 receptors by peripheral administration of the selective agonist (R)alpha-methylhistamine reduced acid secretion in cats, dogs, rats and rabbits, while increasing it in mice. The antisecretory effects were observed against indirect stimuli that act on vagal pathways or on enterochromaffin-like (ECL) cells, such as 2-deoxy-D-glucose, food or pentagastrin, but not against histamine or dimaprit. Inhibitory effects on acid production were observed in rats after central administration of histamine or of H3 receptor agonists. In the conscious rat intragastric administration of (R)alpha-methylhistamine caused gastroprotective effects against the damage induced by absolute ethanol, HCl, aspirin and stress. The mechanism involved seems to be related to the increased mucus production, via nitric oxide-independent mechanisms. Gastroprotective effects against ethanol were also observed after central administration of histamine or its metabolite N(alpha)-methylhistamine, suggesting that brain receptors participate the histamine-mediated effects on gastric functions.

On the myoepithelium of human salivary glands. An immunocytochemical study.

This study investigated the immunocytochemical characteristics of normal myoepithelial cells (MECs) of human major and minor salivary glands using the LSAB method. Other human exocrine glands were used as controls. Immunoreactivity of MECs was observed exclusively with fully differentiated smooth muscle antibodies (a-SMA; SMMS-1; CALP; hCD) and with epithelial markers (cytokeratins) Ck14 and Ck17. This epithelial-muscular immunophenotype was similarly expressed in the MECs of other human exocrine glands used as control. In the salivary MECs, we did not observe evidence for neuroectodermic phenotype (S-100 protein, GFAP, NSE). On the contrary, positivity was observed for S-100 protein in Mecs of control glands (mammary, bronchial and sweat glands). Immunoreaction for extracellular matrix markers (fibronectin, laminin and collagen IV) and vimentin always were negative. Our data show that in normal "non transformed" MECs of the salivary glands the smooth muscle phenotype is in a state of complete differentiation, while the epithelial phenotype expresses only Ck14 and Ck17. This double and simultaneous immunoreactivity represents a differential marker of MECs from the epithelial basal cell (EBCs).

Histamine H(3)-receptor antagonists inhibit gastroprotection by (R)-alpha-methylhistamine in the rat.

(R)-alpha-methylhistamine, a selective agonist of histamine H(3) receptors, is capable of protecting the gastric mucosa against differently acting damaging agents. The objective of the present study was to determine whether H(3) receptors mediate its protective action in the rat. Gastric mucosal lesions were induced intragastrically (i.g.) by 0.6 N HCl, 1 ml rat(-1). (R)-alpha-methylhistamine, 100 mg kg(-1) i.g., substantially reduced the severity of macroscopically and histologically assessed damage caused by concentrated acid. Prior treatment with highly selective H(3)-receptor antagonists, ciproxifan (0.3, 1 and 3 mg kg(-1) i.g.) and clobenpropit (3, 10 and 30 mg kg(-1) i.g.), dose-dependently inhibited the protection exerted by (R)-alpha-methylhistamine up to a complete reversal. When given alone at high doses, both antagonists tended to worsen the HCl-induced histologic damage. During basal conditions, (R)-alpha-methylhistamine, 100 mg kg(-1) i. g., caused a significant increase in titratable acidity of the gastric juice. Prior treatment with ciproxifan (3 mg kg(-1) i.g.) and clobenpropit (30 mg kg(-1) i.g.) did not alter the secretory response to (R)-alpha-methylhistamine. Clobenpropit alone, but not ciproxifan, increased the volume of gastric juice, and both compounds alone had no effect on titratable acid. Present findings support evidence that H(3) receptors are actively involved in the maintenance of gastric mucosal integrity, with no apparent role in the regulation of basal gastric acid secretion.

Famotidine prevents deep histologic lesions induced by 0.6N HCl in rat gastric mucosa: role of parietal cells.

The assessment of the protective actions of H2-receptor antagonists against gastric mucosal lesions by necrotizing agents relies on the gross observation of the gastric mucosa only. We examined the activity of famotidine against 0.6 N HCl-induced damage and the role of parietal cells by light and transmission electron microscopy. Rats received famotidine 0.3-10 mg/kg intragastrically. Sixty minutes later 0.6 N HCl (1 ml/rat) was given and after an additional 30 min the stomachs were removed. Macroscopically visible lesions were measured. Histologic lesions were scored on the basis of the depth. The ultrastructure of parietal cells in the isthmus-neck region was examined. Pretreatment with famotidine resulted in a slight increase of macroscopically visible gastric lesions in response to HCl. While the extent of total histologic damage was not modified, the antisecretory dose significantly reduced only lesions deep within the mucosa. Famotidine alone determined the dose-dependent occurrence of a distinct parietal cell morphological state, suggestive of inhibition of the secretory system. A causal link between the protective effect on the region where parietal cells are located, the percentage of cells shifting to the inhibited morphological state, and the inhibitory effect on acid secretion is proposed.