Autogenous and efficient acceleration of energetic ions upstream of Earth's bow shock.

Earth and its magnetosphere are immersed in the supersonic flow of the solar-wind plasma that fills interplanetary space. As the solar wind slows and deflects to flow around Earth, or any other obstacle, a 'bow shock' forms within the flow. Under almost all solar-wind conditions, planetary bow shocks such as Earth's are collisionless, supercritical shocks, meaning that they reflect and accelerate a fraction of the incident solar-wind ions as an energy dissipation mechanism1,2, which results in the formation of a region called the ion foreshock3. In the foreshock, large-scale, transient phenomena can develop, such as 'hot flow anomalies'4-9, which are concentrations of shock-reflected, suprathermal ions that are channelled and accumulated along certain structures in the upstream magnetic field. Hot flow anomalies evolve explosively, often resulting in the formation of new shocks along their upstream edges5,10, and potentially contribute to particle acceleration11-13, but there have hitherto been no observations to constrain this acceleration or to confirm the underlying mechanism. Here we report observations of a hot flow anomaly accelerating solar-wind ions from roughly 1-10 kiloelectronvolts up to almost 1,000 kiloelectronvolts. The acceleration mechanism depends on the mass and charge state of the ions and is consistent with first-order Fermi acceleration14,15. The acceleration that we observe results from only the interaction of Earth's bow shock with the solar wind, but produces a much, much larger number of energetic particles compared to what would typically be produced in the foreshock from acceleration at the bow shock. Such autogenous and efficient acceleration at quasi-parallel bow shocks (the normal direction of which are within about 45 degrees of the interplanetary magnetic field direction) provides a potential solution to Fermi's 'injection problem', which requires an as-yet-unexplained seed population of energetic particles, and implies that foreshock transients may be important in the generation of cosmic rays at astrophysical shocks throughout the cosmos.

Prompt Response of the Dayside Magnetosphere to Discrete Structures Within the Sheath Region of a Coronal Mass Ejection.

A sequence of discrete solar wind structures within the sheath region of an interplanetary coronal mass ejection on November 6, 2015, caused a series of compressions and releases of the dayside magnetosphere. Each compression resulted in a brief adiabatic enhancement of ions (electrons) driving bursts of electromagnetic ion cyclotron (EMIC; whistler mode chorus) wave growth across the dayside magnetosphere. Fine-structured rising tones were observed in the EMIC wave bursts, resulting in nonlinear scattering of relativistic electrons in the outer radiation belt. Multipoint observations allow us to study the spatial structure and evolution of these sheath structures as they propagate Earthward from L1 as well as the spatio-temporal characteristics of the magnetospheric response. This event highlights the importance of fine-scale solar wind structure, in particular within complex sheath regions, in driving dayside phenomena within the inner magnetosphere.

Electron Bulk Acceleration and Thermalization at Earth's Quasiperpendicular Bow Shock.

Electron heating at Earth's quasiperpendicular bow shock has been surmised to be due to the combined effects of a quasistatic electric potential and scattering through wave-particle interaction. Here we report the observation of electron distribution functions indicating a new electron heating process occurring at the leading edge of the shock front. Incident solar wind electrons are accelerated parallel to the magnetic field toward downstream, reaching an electron-ion relative drift speed exceeding the electron thermal speed. The bulk acceleration is associated with an electric field pulse embedded in a whistler-mode wave. The high electron-ion relative drift is relaxed primarily through a nonlinear current-driven instability. The relaxed distributions contain a beam traveling toward the shock as a remnant of the accelerated electrons. Similar distribution functions prevail throughout the shock transition layer, suggesting that the observed acceleration and thermalization is essential to the cross-shock electron heating.

Relativistic Electrons Produced by Foreshock Disturbances Observed Upstream of Earth's Bow Shock.

Charged particles can be reflected and accelerated by strong (i.e., high Mach number) astrophysical collisionless shock waves, streaming away to form a foreshock region in communication with the shock. Foreshocks are primarily populated by suprathermal ions that can generate foreshock disturbances-large-scale (i.e., tens to thousands of thermal ion Larmor radii), transient (∼5-10 per day) structures. They have recently been found to accelerate ions to energies of several keV. Although electrons in Saturn's high Mach number (M>40) bow shock can be accelerated to relativistic energies (nearly 1000 keV), it has hitherto been thought impossible to accelerate electrons beyond a few tens of keV at Earth's low Mach number (1≤M<20) bow shock. Here we report observations of electrons energized by foreshock disturbances to energies up to at least ∼300 keV. Although such energetic electrons have been previously observed, their presence has been attributed to escaping magnetospheric particles or solar events. These relativistic electrons are not associated with any solar or magnetospheric activity. Further, due to their relatively small Larmor radii (compared to magnetic gradient scale lengths) and large thermal speeds (compared to shock speeds), no known shock acceleration mechanism can energize thermal electrons up to relativistic energies. The discovery of relativistic electrons associated with foreshock structures commonly generated in astrophysical shocks could provide a new paradigm for electron injections and acceleration in collisionless plasmas.

Human globin messenger RNA: importance of cloning for structural analysis.

The sequence of most of the human beta globin messenger RNA and large sections of the alpha globin messenger RNA has been determined. Partly because of genetic polymorphism, it was necessary to clone globin complementary DNA in order to extend the analysis. Purified human fetal globin messenger RNA was isolated and used as a template by reverse transcriptase to produce duplex complementary DNA molecules. These molecules were linked in vitro to plasmid DNA by use of T4 ligase in the presence of Escherichia coli Pol 1. Several colonies transformed by these molecules have been shown to hybridize with labeled human globin complementary RNA.

Waves in interplanetary shocks: a wind/WAVES study.

We describe results from the first statistical study of waveform capture data during 67 interplanetary (IP) shocks with Mach numbers ranging from approximately 1-6. Most of the waveform captures and nearly 100% of the large amplitude waves were in the ramp region. Although solitary waves, Langmuir waves, and ion acoustic waves (IAWs) are all observed in the ramp region of the IP shocks, large amplitude IAWs dominate. The wave amplitude is correlated with the fast mode Mach number and with the shock strength. The observed waves produced anomalous resistivities from approximately 1-856 Omega.m (approximately 10(7) times greater than classical estimates.) The results are consistent with theory suggesting IAWs provide the primary dissipation for low Mach number shocks.

Revisiting the structure of low-Mach number, low-beta, quasi-perpendicular shocks.

A study of the structure of 145 low-Mach number (M ≤ 3), low-beta (ß ≤ 1), quasi-perpendicular interplanetary collisionless shock waves observed by the Wind spacecraft has provided strong evidence that these shocks have large-amplitude whistler precursors. The common occurrence and large amplitudes of the precursors raise doubts about the standard assumption that such shocks can be classified as laminar structures. This directly contradicts standard models. In 113 of the 145 shocks (~78%), we observe clear evidence of magnetosonic-whistler precursor fluctuations with frequencies ~0.1-7 Hz. We find no dependence on the upstream plasma beta, or any other shock parameter, for the presence or absence of precursors. The majority (~66%) of the precursors propagate at ≤45° with respect to the upstream average magnetic field and most (~87%) propagate ≥30° from the shock normal vector. Further, most (~79%) of the waves propagate at least 20° from the coplanarity plane. The peak-to-peak wave amplitudes (δB pk-pk) are large with a range of maximum values for the 113 precursors of ~0.4-13 nT with an average of ~2 nT. When we normalize the wave amplitudes to the upstream averaged magnetic field and the shock ramp amplitude, we find average values of ~40% and ~220%, respectively.

Brief stimulation of the peroneal nerve attenuates the exercise pressor reflex in anaesthetised cats.

We recently demonstrated that applying capsaicin to the common peroneal nerve, thereby activating small diameter afferent neurons, caused a substantial rise in mean arterial pressure (MAP) and heart rate (HR) that lasted approximately 20 min. In addition, this application of capsaicin transiently attenuated the exercise pressor reflex (EPR). The purpose of the current study was to test the hypothesis that stimulating the peroneal nerve at an intensity that activated both myelinated and unmyelinated axons for a short duration (1 min) causes a similar attenuation of the EPR. Cats were anaesthetised with alpha-chloralose and urethane, the popliteal fossa was exposed, and static contraction was induced by stimulating the tibial nerve. The ipsilateral peroneal nerve was cut and placed on a stimulating electrode. Prior to peroneal nerve stimulation, static contraction of the triceps surae muscle for 1 min increased MAP 48+/-8 mmHg and HR 16+/-3 bpm. Electrical stimulation of the central end of the cut peroneal nerve for 1 min (100 x motor threshold; 40 Hz; 0.1 ms) increased MAP and HR by 62+/-11 mmHg and 28+/-4 bpm, respectively. These increases returned to prestimulation levels within 1 min. Two minutes after the peroneal stimulation was stopped, the EPR was markedly reduced as muscle contraction increased MAP and HR by 20+/-4 mmHg and 7+/-2 bpm, respectively. Repeating the muscle contraction approximately 25 min after peroneal stimulation increased MAP and HR by 38+/-8 mmHg and 12+/-2 bpm, indicating some recovery of the EPR. These results show that brief (1 min) electrical stimulation of afferent neurons in the peroneal nerve attenuates the EPR. This supports the hypothesis that strong activation of small diameter afferent neurons stimulates a nervous system mechanism that diminishes the sensory input from skeletal muscle involved in cardiovascular regulation.

Attenuation of the reflex responses to muscle contraction by the coadministration of antagonists to substance P and somatostatin into the dorsal horn.

OBJECTIVE: The aim was to determine if the coadministration of antagonists to substance P and somatostatin into the L7 dorsal horn blunts the reflex cardiovascular responses to static contraction to a greater extent than each antagonist alone. The possibility that this attenuation is mediated by blunting the contraction evoked increases in sympathetic outflow was also tested. METHODS: Using alpha chloralose anaesthetised cats (n = 8), static contraction and stretch of the triceps surae muscle were performed before and after microinjecting (1 microliter) 250 ng of the substance P antagonist, D-Pro2-D-Phe7-D-Trp9-substance P, and the somatostatin antagonist, cyclo(7-amino-heptanoyl-phenylalanyl-D-tryptophyl-lysyl-threonyl-[ benzyl]). The muscle was contracted by electrically stimulating the peripheral end of the cut L7 ventral root. RESULTS: Before injecting the antagonists, static muscle contraction increased mean arterial blood pressure by 40(SEM 6) mm Hg, heart rate by 13(2) beats.min-1, and renal sympathetic nerve activity (RSNA) by 41(7)%. These changes were blunted by the antagonists since the increases in blood pressure, heart rate, and RSNA were reduced to 21(3) mm Hg, 8(1) beats.min-1, and 23(5)%, respectively. In contrast, antagonist administration did not affect the pressor [33(5) v 31(5) mm Hg], heart rate [9(2) v 10(2) beats.min-1], or RSNA [23(4)% v 25(5)%] responses to muscle stretch. Microinjection of 2% lignocaine into the dorsal horn virtually abolished the reflex changes elicited by muscle stretch. CONCLUSIONS: The release of substance P and somatostatin in the spinal cord plays a role in mediating the cardiovascular changes caused by static contraction, but the release of other neurotransmitters/neuromodulators is also involved. The attenuation produced by these antagonists is mediated, at least in part, by reducing sympathetic outflow.

Nucleotide sequence of human G gamma globin messenger RNA.

The nucleotide sequences of the entire coding portion and 3'-untranslated portion of the human G gamma globin mRNA have been determined by direct nucleotide sequence analysis of cloned human G gamma globin cDNAs. These nucleotides sequences have been compared to the previously published sequences of the human beta globin mRNA and A gamma globin mRNA. No differences were detected between the coding sequences of G gamma and A gamma globin mRNAs except for the expected difference at codon No. 136, but a number of differences were detected in the 3'-untranslated sequences of the two mRNAs. Codon usage of G gamma globin mRNA, although similar to that of the related beta globin mRNA, displays a few notable differences such as the use of UUG for leucine and GGA for glycine that are not utilized in beta globin mRNA.

Dorsal horn administration of muscimol abolishes the muscle pressor reflex.

The purpose of this study was to determine the effect of blocking synaptic transmission in the dorsal horn on the cardiovascular responses produced by activation of muscle afferent neurons. Synaptic transmission was blocked by applying the GABA(A) agonist muscimol to the dorsal surface of the spinal cord. Cats were anesthetized with alpha-chloralose and urethane, and a laminectomy was performed. With the exception of the L(7) dorsal root, the dorsal and ventral roots from L(5) to S(2) were sectioned on one side, and static contraction of the ipsilateral triceps surae muscle was evoked by electrically stimulating the peripheral ends of the L(7) and S(1) ventral roots. The dorsal surface of the L(4)--S(3) segments of the spinal cord were enclosed within a "well" created by applying layers of vinyl polysiloxane. Administration of a 1 mM solution of muscimol (based on dose-response data) into this well abolished the reflex pressor response to contraction (change in mean arterial blood pressure before was 47 +/- 7 mmHg and after muscimol was 3 +/- 2 mmHg). Muscle stretch increased mean arterial blood pressure by 30 +/- 8 mmHg before muscimol, but after drug application stretch increased MAP by only 3 +/- 2 mmHg. Limiting muscimol to the L(7) segment attenuated the pressor responses to contraction (37 +/- 7 to 24 +/- 11 mmHg) and stretch (28 +/- 2 to 16 +/- 8 mmHg). These data suggest that the dorsal horn of the spinal cord contains an obligatory synapse for the pressor reflex. Furthermore, these data support the hypothesis that branches of primary afferent neurons, not intraspinal pathways, are responsible for the multisegmental integration of the pressor reflex.

Chemoreflex blunting of hypoxic pulmonary vasoconstriction is vagally mediated.

We investigated the role of the autonomic nervous system in the arterial chemoreceptor attenuation of hypoxic pulmonary vasoconstriction (HPV) using anesthetized dogs. Total pulmonary blood flow (Qt) and left pulmonary blood flow (Ql) were determined using electromagnetic flow probes. Carotid body chemoreceptors were perfused using blood pumped from an extracorporeal circuit containing an oxygenator. Four groups were used: 1) prevagotomy (control), 2) bilateral vagotomy, 3) post-atropine, and 4) post-propranolol. Left lung hypoxia decreased Ql/Qt from 42.9 +/- 2.9 to 28.1 +/- 3.0%, from 41.1 +/- 5.3 to 26.7 +/- 4.2%, from 38.6 +/- 1.3 to 22.2 +/- 2.4%, and from 48.2 +/- 4.2 to 28.5 +/- 3.7% in the four groups, respectively. Chemoreceptor stimulation during unilateral hypoxia increased Ql/Qt from 28.1 +/- 3.0 to 39.1 +/- 4.9% and from 28.5 +/- 3.7 to 40.6 +/- 3.7% in the control and propranolol groups. However, chemoreceptor stimulation had no effect on Ql/Qt during left lung hypoxia after vagotomy or atropine, as Ql/Qt went from 26.7 +/- 4.2 to 29.3 +/- 5.2% and from 22.2 +/- 2.4 to 24.1 +/- 1.5% in groups 2 and 3, respectively. Because chemoreceptor stimulation did not affect HPV in groups 2 and 3, we conclude that the chemoreceptor attenuation of HPV is mediated by the parasympathetic nervous system.

Excitatory amino acid concentrations in the spinal dorsal horn of cats during muscle contraction.

In anesthetized cats, static hindlimb muscle contraction reflexly increases mean arterial pressure (MAP) and heart rate (HR). Pharmacological and immunohistochemical evidence suggests that excitatory amino acids are involved in the spinal transmission of this reflex. Using microdialysis and high-performance liquid chromatography technology, we tested the hypothesis that static contraction of the triceps surae muscle increases the extracellular concentration of glutamate (Glu) and aspartate (Asp) at the L7 level of the dorsal horn of the spinal cord. With the exception of the L7 dorsal root, the L5-S2 dorsal and ventral roots were cut ipsilateral to the contracting muscle. After the insertion of microdialysis probes and a 3-h recovery period, a 2-min static contraction was electrically evoked. MAP and HR increased by 53 +/- 8 mmHg and 20 +/- 4 beats/min. The concentration of Glu increased from 324 +/- 59 to 857 +/- 80 nM, whereas Asp increased from 199 +/- 57 to 499 +/- 113 nM. These results were repeatable, in that Glu and Asp rose by similar amounts in two subsequent contractions. In both of these latter contractions, MAP and HR were also significantly increased. By contrast, in a subset of cats whose L7 dorsal roots were cut after the first contraction, neither MAP, HR, Glu, nor Asp was significantly increased over baseline levels. These data demonstrate that static contraction of the hindlimb increases the extracellular concentration of Glu and Asp in the dorsal horn. In summary, the results from this study are in agreement with previous findings suggesting that excitatory amino acids are involved in the spinal transmission of sensory information from the hindlimb muscle.

Cardiovascular and renal nerve responses to static muscle contraction of decerebrate rabbits.

The purpose of this study was to determine whether the biphasic arterial blood pressure responses elicited by static muscle contraction of decerebrate rabbits are mediated, at least in part, by an initial decrease and a subsequent increase in sympathetic outflow. Renal sympathetic nerve activity (RSNA) was used as an index of sympathetic outflow. Static contraction of the triceps surae muscle (n = 14) initially decreased mean arterial blood pressure (MAP) -20 +/- 3 mmHg and heart rate (HR) -15 +/- 5 beats/min (nadir values). After this initial decrease, MAP increased 12 +/- 2 mmHg (peak increase) above baseline and there was a tendency for HR to be elevated (6 +/- 3 beats/min). The changes in RSNA during muscle contraction (n = 6) mirrored the nadir and peak responses of MAP (-50 +/- 9 and 32 +/- 11%). Muscle stretch (n = 11) also evoked similar nadir and peak responses of MAP (-20 +/- 5 and 9 +/- 1 mmHg), HR (-17 +/- 7 and 3 +/- 3 beats/min), and RSNA (-43 +/- 9 and 46 +/- 15%). These data suggest that the initial depressor and subsequent pressor responses elicited by skeletal muscle contraction and stretch are mediated, at least in part, by biphasic changes in sympathetic outflow.

Effect of skeletal muscle fiber type on the pressor response evoked by static contraction in rabbits.

The purpose of this study was to determine whether the reflex hemodynamic responses to static contraction of predominately glycolytic muscle are greater than the changes elicited by primarily oxidative muscle. Low-frequency electrical stimulation (continuous 21 days) of the tibial nerve of one hindlimb of adult rabbits converted the metabolic characteristics of the predominately glycolytic gastrocnemius to a muscle that was primarily oxidative. After 21 days of stimulation, the rabbits were decerebrated, and static contraction of the glycolytic muscle (unstimulated gastrocnemius) initially decreased heart rate (HR; -16 +/- 3 beats/min) and mean arterial pressure (MAP; -17 +/- 3 mmHg). Thereafter, MAP increased 13 +/- 3 mmHg above baseline. Static contraction of the oxidative muscle (stimulated gastrocnemius) produced similar decreases in HR and MAP (-12 +/- 4 beats/min and -12 +/- 3 mmHg, respectively). However, the subsequent increase in MAP (8 +/- 3 mmHg; above baseline) was less than that evoked by contraction of the glycolytic muscle. The responses evoked by stretch of each muscle and high-intensity electrical stimulation were the same, indicating that the afferents from the muscle were not destroyed by the chronic-stimulation technique. These results support the hypothesis that metabolic by-products play a role in the pressor response to static contraction of skeletal muscle. In addition, these data confirm that contraction of predominately oxidative muscle can evoke a reflex pressor response, albeit smaller than the change elicited from primarily glycolytic muscle.

Segmental effect of NMDA block in the dorsal horn on the pressor reflex.

The purpose of this study was to examine the influence of NMDA receptor blockade in the dorsal horn of adjacent spinal segments as it pertains to the pressor reflex evoked by static contraction and stretch of skeletal muscle. In this preparation, cats were anesthetized and the afferent fibers mediating the pressor reflex entered the spinal cord via the L7 dorsal root. Blockade of dorsal horn NMDA receptors at L6 and L7 attenuated the pressor reflex evoked by static contraction and muscle stretch. However, NMDA block in the L6 dorsal horn alone failed to alter the peak increase in MAP produced by static contraction and muscle stretch, but the initial pressor response evoked by static contraction was attenuated. These data support the hypothesis that the pressor reflex is partially mediated by activation of NMDA receptors in the dorsal horn, and this occurs at multiple spinal segments. Further, these data suggest that activation of NMDA receptors plays an important role in initiating the rise in arterial pressure produced by static contraction of skeletal muscle.

Multiplicity of the afferent pathways mediating the exercise pressor reflex.

The cardiovascular responses to isometric contraction of the triceps surae muscle of one leg were determined before and after transecting the ipsilateral L7 or L6 and S1 spinal roots. Sectioning only the L7 spinal root slightly attenuated the pressor, but not the heart rate response induced by skeletal muscle contraction, while cutting the L6 and S1 spinal roots (L7 intact) had no effect on the cardiovascular changes. This indicates that there is multiplicity in neural afferent pathways that mediate the exercise pressor reflex.

Cardiovascular effects elicited by central administration of physostigmine via M2 muscarinic receptors in conscious cats.

The cardiovascular effects of an intracerebroventricular (i.c.v.) injection of physostigmine were studied using conscious cats. Physostigmine (5-25 micrograms: 5 microliters) caused a dose-dependent increase in mean arterial pressure (MAP) and heart rate (HR). The highest dose (25 micrograms) increased MAP and HR by 32 +/- 3 mmHg and 45 +/- 5 beats/min, respectively (n = 5). Pre-administration of the muscarinic receptor antagonist, atropine (25 micrograms; i.c.v.) blocked the effects of physostigmine (25 micrograms; i.c.v.). Also, the pre-administration of the M2 muscarinic antagonist, methoctramine (25 micrograms; i.c.v.), antagonized the cardiovascular effects of physostigmine without altering the baseline variables. However, the M1 muscarinic antagonist, pirenzepine (100 micrograms; i.c.v.) did not alter baseline MAP or HR, and also failed to inhibit the cardiovascular responses to physostigmine. Similarly, the M3 muscarinic blocker, 4-diphenyl-acetoxy-N-methylpiperidine methiodide (50 micrograms; i.c.v.), neither changed baseline cardiovascular variables nor blocked the effects of physostigmine. When the same cats were anesthetized with intravenous injection of sodium pentobarbital (25-30 mg/kg), physostigmine (25 micrograms; i.c.v.) evoked a decrease in MAP and HR of 13 +/- 6 mmHg and 15 +/- 6 bpm, respectively (n = 5). These results demonstrate that the increases in MAP and HR to the i.c.v. administration of physostigmine in conscious cats are possibly mediated through stimulation of central M2 muscarinic receptors. In addition, anesthesia reverses the effects elicited by the central administration of physostigmine to a decrease in MAP and HR.

Spinal cholinergic inhibition of the pressor response to skeletal muscle activation.

The purpose of this study was to delineate the role of the cholinergic pathway within the spinal cord in the reflex cardiovascular responses to muscle activity. Based on dose-response experiments, we microdialyzed a 0.1 mM solution of the acetylcholinesterase inhibitor neostigmine into the L7 level of the dorsal horn of anesthetized cats to determine its effects on the mean arterial blood pressure (MAP) and heart rate (HR) responses to static muscle contraction or passive stretch. The peak responses to 1-min contractions and stretches were reduced from control levels after 1 h of drug administration. In four experiments, the cardiovascular responses returned to control levels after a 2-h recovery period. Perfusion of the cholinergic receptor antagonist atropine accentuated the peak MAP response to muscle contraction. By contrast, atropine administration had no effect on the peak MAP adjustment to passive muscle stretch. These data support the hypothesis that increased acetylcholine (ACh) concentrations in the spinal cord inhibit the reflex cardiovascular responses to static muscle contraction. Further, the results suggest that the spinal cholinergic system is activated by metabolic changes in skeletal muscle, but likely unaffected by mechanical muscle changes.

Spinal cholinergic inhibition of the pressor response to muscle activation is mediated by muscarinic, but not nicotinic, receptors.

This study examined the influence of spinal muscarinic and nicotinic receptors on the cardiovascular adjustments to skeletal muscle activation in anesthetized cats. Microdialyzing into the L(7) dorsal horn increasing doses of the muscarinic receptor agonist bethanechol, but not the nicotinic receptor antagonist mecamylamine, reduced increases in mean arterial pressure (MAP) and heart rate (HR) during hindlimb contraction or passive stretch. Atropine administration accentuated the cardiovascular responses during contraction, but not during passive stretch. These data indicate that muscarinic, but not nicotinic, receptors at the dorsal horn level blunt the pressor response to muscle activity. Further, the data suggest that the two neural pathways involved in muscle contraction or stretch are anatomically distinct.